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Relativistic Sweet-Parker Current Sheet and Its Macroscopic Evolution. The problem of the relativistic Sweet-Parker current sheet is investigated, incorporating the effects of resistivity and thermal inertia. The scaling laws of the steady-state current sheet are obtained, and generalizations are carried out to include... | [
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The Impact of Pair-instability Mass Loss on the Binary Black Hole Mass Distribution. A population of binary black hole mergers has now been observed in gravitational waves by Advanced LIGO and Virgo. The masses of these black holes appear to show evidence for a pileup between 30 and 45 M ⊙ and a cutoff above ∼45 M ⊙. O... | [
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Quantifying the Propagation of Fast Coronal Mass Ejections from the Sun to Interplanetary Space by Combining Remote Sensing and Multi-point In Situ Observations. In order to have a comprehensive view of the propagation and evolution of coronal mass ejections (CMEs) from the Sun to deep interplanetary space beyond 1 au,... | [
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Magnetic Structures at the Boundary of the Closed Corona: A Semi-automated Study of S-Web Morphology. Interchange reconnection is thought to play an important role in driving the dynamics of the slow solar wind. To understand the details of this process, it is important to catalog the various magnetic structures that a... | [
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Jellyfish: Ram Pressure Stripping As a Diagnostic Tool in Studies of Cluster Collisions. Prompted by the discovery of A1758N_JFG1, a spectacular case of ram pressure stripping (RPS) in the galaxy cluster A1758N, we investigate the properties of other galaxies suspected to undergo RPS in this equal-mass, post-collision ... | [
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Probing CO and N<SUB>2</SUB> Snow Surfaces in Protoplanetary Disks with N<SUB>2</SUB>H<SUP>+</SUP> Emission. Snowlines of major volatiles regulate the gas and solid C/N/O ratios in the planet-forming midplanes of protoplanetary disks. Snow surfaces are the 2D extensions of snowlines in the outer disk regions, where rad... | [
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Hunting Young White Dwarfs at the Center of Planetary Nebulae. We present Gemini-South observations of nine faint and extended planetary nebulae (PNe). Using direct images taken with the spectrograph Gemini-South multi-object spectrograph (GMOS), we built the (u\prime -g\prime ) versus (g\prime -r\prime ) diagrams of t... | [
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X-Ray Monitoring of the Magnetar CXOU J171405.7-381031 in Supernova Remnant CTB 37B. We present the results of our 8 yr X-ray monitoring campaign on CXOU J171405.7-381031, the magnetar associated with the faint supernova remnant (SNR) CTB 37B. It is among the youngest by inferred spin-down age, and most energetic in sp... | [
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Detailed Chemical Composition and Orbit of the Newly Discovered Globular Cluster FSR 1758: Implications for the Accretion of the Sequoia Dwarf Galaxy onto the Milky Way. We present detailed chemical abundances, radial velocity, and orbital parameters for FSR 1758, a recently discovered massive cluster in the direction ... | [
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Chemical Abundance Analysis of Tucana III, the Second r-process Enhanced Ultra-faint Dwarf Galaxy. We present a chemical abundance analysis of four additional confirmed member stars of Tucana III, a Milky Way satellite galaxy candidate in the process of being tidally disrupted as it is accreted by the Galaxy. Two of th... | [
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"http://astrothesaurus.org/uat/1108",
"http://astrothesaurus.org/uat/1324",
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Distances to Galactic OB Stars: Photometry versus Parallax. For application to surveys of interstellar matter and Galactic structure, we compute new spectrophotometric distances to 139 OB stars frequently used as background targets for UV spectroscopy. Many of these stars have updated spectral types and digital photome... | [
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A Catalog of Hyper-luminous X-Ray Sources and Intermediate-mass Black Hole Candidates out to High Redshifts. Hyper-luminous X-ray sources (HLXs; L X > 1041 erg s-1) are off-nuclear X-ray sources in galaxies and strong candidates for intermediate-mass black holes (IMBHs). We have constructed a sample of 169 HLX candi... | [
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"http://astrothesaurus.org/uat/16",
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"http://astrothesaurus.org/uat/1569",
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Earth as an Exoplanet: A Two-dimensional Alien Map. Resolving spatially varying exoplanet features from single-point light curves is essential for determining whether Earth-like worlds harbor geological features and/or climate systems that influence habitability. To evaluate the feasibility and requirements of this spa... | [
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Active Asteroid (6478) Gault: A Blue Q-type Surface below the Dust?. We present near-infrared spectroscopy of the sporadically active asteroid (6478) Gault collected on the 3 m NASA/Infrared Telescope Facility observatory in late 2019 March/early April. Long-exposure imaging with the 0.5 m Near Earth Environment Monito... | [
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Fermi-LAT Stacking Analysis Technique: An Application to Extreme Blazars and Prospects for their CTA Detection. We present a likelihood profile stacking technique based on the Fermi-Large Area Telescope (LAT) data to explore the γ-ray characteristics of Fermi-LAT undetected astrophysical populations. The pipeline is ap... | [
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A Mass-accreting Gamma Doradus Pulsator with a Synchronized Core in Kepler Eclipsing Binary KIC 7385478. The short-period (P ≈ 1.7 days), Algol-type eclipsing binary KIC 7385478 consists of an F-type primary star (M 1 ≈ 1.71M ⊙) and an evolved K-type secondary (M 2 ≈ 0.37M ⊙). We study the variability of the Kepler lig... | [
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"http://astrothesaurus.org/uat/2101"
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Pure Rotational Spectrum of CN<SUP>+</SUP>. The pure rotational spectrum of the elusive CN+ cation has been observed for the first time using a cryogenic ion trap apparatus and applying an action spectroscopy scheme. For the 12C14N+ species, the three lowest rotational transitions have been observed, each of which exhi... | [
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"http://astrothesaurus.org/uat/2073",
"http://astrothesaurus.org/uat/2004",
"http://astrothesaurus.org/uat/2058"
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Atomic Hydrogen in Star-forming Galaxies at Intermediate Redshifts. We have used the upgraded Giant Metrewave Radio Telescope to carry out a deep (117 on-source hours) L-band observation of the Extended Groth Strip, to measure the average neutral hydrogen (H I) mass and median star formation rate (SFR) of star-forming ... | [
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"http://astrothesaurus.org/uat/1346",
"http://astrothesaurus.org/uat/734"
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"http://astrothesaurus.org/uat/1379",
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Distinct Properties of the Radio Burst Emission from the Magnetar XTE J1810-197. XTE J1810-197 (PSR J1809-1943) was the first magnetar that was found to emit transient radio emission. It has recently undergone another radio and high-energy outburst. This is only the second radio outburst that has been observed from thi... | [
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Time-varying Polarized Gamma-Rays from GRB 160821A: Evidence for Ordered Magnetic Fields. GRB 160821A is the third most energetic gamma-ray burst observed by the Fermi gamma-ray space telescope. Based on the observations made by the Cadmium Zinc Telluride Imager on board AstroSat, here we report the most conclusive evi... | [
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Long-lived Eccentricities in Accretion Disks. Accretion disks can be eccentric: they support m = 1 modes that are global and slowly precessing. But whether the modes remain trapped in the disk—and hence are long-lived—depends on conditions at the outer edge of the disk. Here we show that in disks with realistic boundar... | [
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Do Androids Dream of Magnetic Fields? Using Neural Networks to Interpret the Turbulent Interstellar Medium. The interstellar medium (ISM) of galaxies is composed of a turbulent magnetized plasma. In order to quantitatively measure relevant turbulent parameters of the ISM, a wide variety of statistical techniques and me... | [
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Limits on the Weak Equivalence Principle and Photon Mass with FRB 121102 Subpulses. Fast radio bursts (FRBs) are short-duration (∼millisecond) radio transients with cosmological origin. The simple sharp features of the FRB signal have been utilized to probe two fundamental laws of physics, namely, testing Einstein’s we... | [
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SN 2018hna: 1987A-like Supernova with a Signature of Shock Breakout. High-cadence ultraviolet, optical, and near-infrared photometric and low-resolution spectroscopic observations of the peculiar Type II supernova (SN) 2018hna are presented. The early-phase multiband light curves (LCs) exhibit the adiabatic cooling env... | [
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Role of Planetary Obliquity in Regulating Atmospheric Escape: G-dwarf versus M-dwarf Earth-like Exoplanets. We present a three-species (H+, O+ and e-) multi-fluid magnetohydrodynamic model, endowed with the requisite upper-atmospheric chemistry, that is capable of accurately quantifying the magnitude of oxygen ion loss... | [
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Lunar Xenon and the Origin of the Indigenous Component. Lunar indigenous Xe isotopic abundances provide crucial information on relationships not only between gas reservoirs in the solar protoplanetary disk but also regarding planetary fractionation processes and possible space weather effects due to an active young Sun... | [
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CHIME/FRB Detection of the Original Repeating Fast Radio Burst Source FRB 121102. We report the detection of a single burst from the first-discovered repeating fast radio burst (FRB) source, FRB 121102, with the Canadian Hydrogen Intensity Mapping Experiment (CHIME) telescope, which operates in the frequency band 400-8... | [
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Dynamical Confirmation of a Black Hole in MAXI J1820+070. We present time-resolved 10.4 m Gran Telescopio Canarias and 4.2 m William Herschel Telescope intermediate resolution spectroscopy of the X-ray transient MAXI J1820+070 (=ASASSN-18ey) obtained during its decline to the quiescent state. Cross-correlation of the 2... | [
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Detection of Crystalline and Fine-grained Calcic Plagioclases on Vesta. Plagioclase feldspars are among the most prevalent minerals in the solar system, and are present in many chondritic and achondritic meteorite families. Nevertheless, spectral features of plagioclases have never been unambiguously and directly obser... | [
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Discovery of a Very Hot Phase of the Milky Way Circumgalactic Medium with Non-solar Abundance Ratios. We present the discovery of a very hot gas phase of the Milky Way circumgalactic medium (CGM) at T ≈ 107 K, using deep XMM-Newton Reflection Grating Spectrometer observations of the blazar 1ES 1553+113. The hot gas, co... | [
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The Tidal Disruption of Sun-like Stars by Massive Black Holes. We present the first simulations of the tidal disruption of stars with realistic structures and compositions by massive black holes (BHs). We build stars in the stellar evolution code MESA and simulate their disruption in the 3D adaptive-mesh hydrodynamics ... | [
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On the Diversity of Fallback Rates from Tidal Disruption Events with Accurate Stellar Structure. The tidal disruption of stars by supermassive black holes (SMBHs) can be used to probe the SMBH mass function, the properties of individual stars, and stellar dynamics in galactic nuclei. Upcoming missions will detect thous... | [
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Unprecedented Near-infrared Brightness and Variability of Sgr A*. The electromagnetic counterpart to the Galactic center supermassive black hole, Sgr A*, has been observed in the near-infrared for over 20 yr and is known to be highly variable. We report new Keck Telescope observations showing that Sgr A* reached much b... | [
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The First Detection of <SUP>13</SUP>C<SUP>17</SUP>O in a Protoplanetary Disk: A Robust Tracer of Disk Gas Mass. Measurements of the gas mass are necessary to determine the planet formation potential of protoplanetary disks. Observations of rare CO isotopologues are typically used to determine disk gas masses; however, ... | [
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A Kinematically Cold Structure of Candidate Young OB Stars toward the Anticenter. We combine Galaxy Evolution Explorer and Gaia DR2 catalogs to track star formation in the outskirts of our Galaxy. Using photometry, proper motions, and parallaxes we identify a structure of ∼300 OB-type candidates located between 12 and ... | [
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First Sub-parsec-scale Mapping of Magnetic Fields in the Vicinity of a Very-low-luminosity Object, L1521F-IRS. L1521F is found to be forming multiple cores and it is cited as an example of the densest core with an embedded VeLLO in a highly dynamical environment. We present the core-scale magnetic fields (B-fields) in ... | [
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Double Neutron Star Mergers from Hierarchical Triple-star Systems. The isolated binary evolution model for merging neutron stars (NSs) involves processes such as mass transfer, common-envelope evolution, and natal kicks, all of which are poorly understood. Also, the predicted NS-NS merger rates are typically lower than... | [
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The Frequency-dependent Behavior of Subpulse Drifting. I. Carousel Geometry and Emission Heights of PSR B0031-07. The carousel model of pulsar emission attributes the phenomenon of subpulse drifting to a set of discrete sparks located very near the stellar surface rotating around the magnetic axis. Here, we investigate... | [
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Metal Abundances and Star Formation Rates of Emission-line Galaxies in and around the Boötes Void. We explore the possible dependencies of galaxy metal abundance and star formation rate (SFR) on local environment, focusing on the volume of space in and around the Boötes Void. Our sample of star-forming galaxies comes f... | [
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A Search for Cosmic-Ray Proton Anisotropy with the Fermi Large Area Telescope. The Fermi Large Area Telescope (LAT) has amassed a large data set of primary cosmic-ray protons throughout its mission. In fact, it is the largest set of identified cosmic-ray protons ever collected at this energy. The LAT’s wide field of vi... | [
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Variations in α-element Ratios Trace the Chemical Evolution of the Disk. It is well established that the chemical structure of the Milky Way exhibits a bimodality with respect to the α-enhancement of stars at a given [Fe/H]. This has been studied largely based on a bulk α abundance, computed as a summary of several ind... | [
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"http://astrothesaurus.org/uat/1050",
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Detection and Timing of Gamma-Ray Pulsations from the 707 Hz Pulsar J0952-0607. The Low-Frequency Array radio telescope discovered the 707 Hz binary millisecond pulsar (MSP) J0952-0607 in a targeted radio pulsation search of an unidentified Fermi gamma-ray source. This source shows a weak energy flux of F γ = 2.6 × 1... | [
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The Eruption of Outer Spine-like Loops Leading to a Double-stage Circular-ribbon Flare. Circular-ribbon flares occur in a confined magnetic structure, but can also be associated with coronal mass ejections (CMEs) when a filament embedded under the fan erupts. Here we study an M8.7 circular-ribbon flare (SOL2014-12-17T0... | [
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"http://astrothesaurus.org/uat/1496",
"http://astrothesaurus.org/uat/1503"
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EVR-CB-001: An Evolving, Progenitor, White Dwarf Compact Binary Discovered with the Evryscope. We present EVR-CB-001, the discovery of a compact binary with an extremely low-mass (0.21 ± 0.05M ⊙) helium core white dwarf progenitor (pre-He WD) and an unseen low-mass (0.32 ± 0.06M ⊙) helium white dwarf (He WD) companion.... | [
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"http://astrothesaurus.org/uat/288",
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Modeling Mg II During Solar Flares. I. Partial Frequency Redistribution, Opacity, and Coronal Irradiation. The Interface Region Imaging Spectrograph has routinely observed the flaring Mg II near-ultraviolet (NUV) spectrum, offering excellent diagnostic potential and a window into the location of energy deposition. A nu... | [
"http://astrothesaurus.org/uat/1496",
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"http://astrothesaurus.org/uat/1982",
"http://astrothesaurus.org/uat/1965",
"http://astrothesaurus.org/uat/1967",
"http://astrothesaurus.org/uat/1479",
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"Near ultraviolet astronomy",
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Into the Darkness: Classical and Type II Cepheids in the Zona Galactica Incognita. The far side of the Milky Way’s disk is one of the most concealed parts of the known universe due to extremely high interstellar extinction and point-source density toward low Galactic latitudes. Large time-domain photometric surveys ope... | [
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"http://astrothesaurus.org/uat/368",
"http://astrothesaurus.org/uat/841",
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Inverse Compton Cascades in Pair-producing Gaps: Effects of Triplet Pair Production. Inverse Compton-pair cascades are initiated when gamma-rays are absorbed on an ambient soft photon field to produce relativistic pairs, which in turn up-scatter the same soft photons to produce more gamma-rays. If the Compton scatterin... | [
"http://astrothesaurus.org/uat/17",
"http://astrothesaurus.org/uat/1119"
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Sculpting Eccentric Debris Disks with Eccentric Gas Rings. Many debris disks seen in scattered light have shapes that imply their dust grains trace highly eccentric, apsidally aligned orbits. Apsidal alignment is surprising, especially for dust. Even when born from an apse-aligned ring of parent bodies, dust grains hav... | [
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"http://astrothesaurus.org/uat/500",
"http://astrothesaurus.org/uat/239",
"http://astrothesaurus.org/uat/235",
"http://astrothesaurus.org/uat/363",
"http://astrothesaurus.org/uat/238"
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Time-reversed Gamma-Ray Burst Light-curve Characteristics as Transitions between Subluminal and Superluminal Motion. We introduce a simple model to explain the time-reversed and stretched residuals in gamma-ray burst (GRB) pulse light curves. In this model an impactor wave in an expanding GRB jet accelerates from sublu... | [
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The Radial Distribution of Dust Particles in the HL Tau Disk from ALMA and VLA Observations. Understanding planet formation requires one to discern how dust grows in protoplanetary disks. An important parameter to measure in disks is the maximum dust grain size present. This is usually estimated through measurements of... | [
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The Analogous Structure of Accretion Flows in Supermassive and Stellar Mass Black Holes: New Insights from Faded Changing-look Quasars. Despite their factor of ∼108 difference in black hole mass, several lines of evidence suggest possible similarities between black hole accretion flows in active galactic nuclei (AGN) a... | [
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Evidence for Inside-out Galaxy Growth and Quenching of a z ∼ 2 Compact Galaxy From High-resolution Molecular Gas Imaging. We present high spatial resolution imaging of the CO(1-0) line from the Karl G. Jansky Very Large Array of COSMOS 27289, a massive, compact star-forming galaxy (SFG) at z = 2.234. This galaxy was se... | [
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High-resolution Optical Spectroscopy of Stars in the Sylgr Stellar Stream. We observe two metal-poor main-sequence stars that are members of the recently discovered Sylgr stellar stream. We present radial velocities, stellar parameters, and abundances for 13 elements derived from high-resolution optical spectra collect... | [
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Mutual Neutralization in Li<SUP>+</SUP>-D<SUP>-</SUP> Collisions: A Combined Experimental and Theoretical Study. We present a combined experimental and theoretical study of the mutual neutralization (MN) process in collisions of lithium ions (Li+) with deuterium anions (D-) at collision energies below 1 eV. We employ a... | [
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Infrared Interferometric Three-dimensional Diagnosis of the Atmospheric Dynamics of the AGB Star R Dor with VLTI/AMBER. The mechanism of mass loss in late evolutionary stages of low- and intermediate-mass stars is not yet well understood. Therefore, it is crucial to study the dynamics of the region within a few R ⋆, wh... | [
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On the Relation between Flare and CME during GLE-SEP and Non-GLE-SEP Events. Association of solar flares and coronal mass ejections (CMEs) with ground-level enhancement (GLE) is a recognized fact, but questions arise when a similar association is observed for non-GLEs. In this respect, we carry out a detailed study of ... | [
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Changes in Solar Rotation over Two Solar Cycles. We use helioseismic data from ground- and space-based instruments to analyze how solar rotation has changed since the beginning of solar Cycle 23 with emphasis on studying the differences between Cycles 23 and 24. We find that the nature of solar rotation is indeed diffe... | [
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New Spatially Resolved Imaging of the SR 21 Transition Disk and Constraints on the Small-grain Disk Geometry. We present new 0.6-4 μm imaging of the SR 21 transition disk from Keck/NIRC2 and Magellan/MagAO. The protoplanetary disk around SR 21 has a large (∼30-40 au) clearing first inferred from its spectral energy dis... | [
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Heliosheath Properties Measured from a Voyager 2 to Voyager 1 Transient. In mid-2012, a global merged interaction region (GMIR) observed by Voyager 2 crossed through the heliosheath and collided with the heliopause, generating a pressure pulse that propagated into the very local interstellar medium. The effects of the ... | [
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Modeling UV Radiation Feedback from Massive Stars. III. Escape of Radiation from Star-forming Giant Molecular Clouds. Using a suite of radiation hydrodynamic simulations of star cluster formation in turbulent clouds, we study the escape fraction of ionizing (Lyman continuum) and non-ionizing (FUV) radiation for a wide ... | [
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The Implications of Local Fluctuations in the Galactic Midplane for Dynamical Analysis in the Gaia Era. Orbital properties of stars, computed from their six-dimensional phase-space measurements and an assumed Galactic potential, are used to understand the structure and evolution of the Galaxy. Stellar actions, computed... | [
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Stereoscopic Observations of an Erupting Mini-filament-driven Two-sided-loop Jet and the Applications for Diagnosing a Filament Magnetic Field. Ubiquitous solar jets or jet-like activities are generally regarded as an important source of energy and mass input to the upper solar atmosphere and the solar wind. However, t... | [
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Dynamical Masses for the Hyades Binary 80 Tauri. The empirical mass-luminosity relation in the Hyades cluster rests on dynamical mass determinations for five binary systems, of which one is eclipsing and the other four are visual or interferometric binaries. The last one was identified and first measured more than 20 y... | [
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Multiband Optical Light Curves of Black-widow Pulsars. We collect new and archival optical observations of nine “black-widow” millisecond pulsar binaries. New measurements include direct imaging with the Keck, Gemini-S, MDM, and Las Cumbres Observatory 2 m telescopes. This is supplemented by synthesized colors from Kec... | [
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The Fundamental Vibrational Frequencies and Spectroscopic Constants of the Dicyanoamine Anion, NCNCN<SUP>-</SUP> (C<SUB>2</SUB>N<SUB>3</SUB> <SUP>-</SUP>): Quantum Chemical Analysis for Astrophysical and Planetary Environments. Detecting anions in space has relied on a strong collaboration between theoretical and labor... | [
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A Prospective New Diagnostic Technique for Distinguishing Eruptive and Noneruptive Active Regions. Active regions are the source of the majority of magnetic flux rope ejections that become coronal mass ejections (CMEs). To identify in advance which active regions will produce an ejection is key for both space weather p... | [
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Redshift Horizon for Detecting the First Galaxies in Far-infrared Surveys. We explore the possibility of detecting the first galaxies with the next generation of space-based far-infrared (FIR) telescopes by applying an analytical model of primordial dust emission. Our results indicate that FIR/submillimeter sources at ... | [
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A Parameter Space Exploration of Galaxy Cluster Mergers. II. Effects of Magnetic Fields. The hot intracluster plasma in clusters of galaxies is weakly magnetized. Mergers between clusters produce gas compression and motions that can increase the magnetic field strength. In this work, we perform high-resolution nonradia... | [
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Impact of Cosmic-Ray Feedback on Accretion and Chemistry in Circumstellar Disks. We use the gas-grain chemistry code UCLCHEM to explore the impact of cosmic-ray feedback on the chemistry of circumstellar disks. We model the attenuation and energy losses of the cosmic rays as they propagate outward from the star and als... | [
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A DECam Search for Explosive Optical Transients Associated with IceCube Neutrino Alerts. In this work, we investigate the likelihood of association between real-time, neutrino alerts with teraelectronvolt to petaelectronvolt energy from IceCube and optical counterparts in the form of core-collapse supernovae (CC SNe). ... | [
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Constraints on Gamma-Ray and Neutrino Emission from NGC 1068 with the MAGIC Telescopes. Starburst galaxies and star-forming active galactic nuclei are among the candidate sources thought to contribute appreciably to the extragalactic gamma-ray and neutrino backgrounds. NGC 1068 is the brightest of the star-forming gala... | [
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Validating Time-Distance Helioseismic Inversions for Nonseparable Subsurface Profiles of an Average Supergranule. Supergranules are divergent 30 Mm-sized cellular flows observed everywhere at the solar photosphere. Their place in the hierarchy of convective structures and their origin remain poorly understood. Estimati... | [
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Turbulence Dynamo in the Stratified Medium of Galaxy Clusters. The existence of microgauss magnetic fields in galaxy clusters has been established through observations of synchrotron radiation and Faraday rotation. They are conjectured to be generated via small-scale dynamo by turbulent flow motions in the intracluster... | [
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Brown Dwarf Atmospheres as the Potentially Most Detectable and Abundant Sites for Life. We show that the total habitable volume in the atmospheres of cool brown dwarfs with effective temperatures of ∼250-350 K is possibly larger by 2 orders of magnitude than that of Earth-like planets. We also study the role of aerosol... | [
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Search for Eccentric Binary Black Hole Mergers with Advanced LIGO and Advanced Virgo during Their First and Second Observing Runs. When formed through dynamical interactions, stellar-mass binary black holes (BBHs) may retain eccentric orbits (e > 0.1 at 10 Hz) detectable by ground-based gravitational-wave detectors.... | [
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Three-dimensional Density Structure of a Solar Coronal Streamer Observed by SOHO/LASCO and STEREO/COR2 in Quadrature. Helmet streamers are a prominent manifestation of magnetic structures with current sheets in the solar corona. These large-scale structures are regions with high plasma density, overlying active regions... | [
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A Flaring AGN in a ULIRG Candidate in Stripe 82. We report the discovery of a mid-infrared variable AGN that is hosted by an ultraluminous infrared galaxy (ULIRG) in the Sloan Stripe 82 field. WISE J030654.88+010833.6 is a red, extended galaxy, which we estimate to be at a photometric redshift of 0.28 ≤ z ≤ 0.31, based... | [
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Turbulence Driven by Stellar Jets, the Possibility and the Efficiency. We investigate the feedback of the stellar jets on the surrounding interstellar gas based on 2D and 3D simulations applying HD and MHD modules of the PLUTO 4.2 code. The main question we address is whether the stellar jet can be considered as a turb... | [
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Synchrotron Self-Compton as a Likely Mechanism of Photons beyond the Synchrotron Limit in GRB 190114C. GRB 190114C, a long and luminous burst, was detected by several satellites and ground-based telescopes from radio wavelengths to GeV gamma-rays. In the GeV gamma-rays, the Fermi Large Area Telescope detected 48 photon... | [
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The Evolution of O I over 3.2 < z < 6.5: Reionization of the Circumgalactic Medium. We present a survey for metal absorption systems traced by neutral oxygen over 3.2 < z < 6.5. Our survey uses Keck/ESI and VLT/X-Shooter spectra of 199 QSOs with redshifts up to 6.6. In total, we detect 74 O I absorbers, of ... | [
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Can Reverberation-measured Quasars Be Used for Cosmology?. Quasars have been proposed as a new class of standard candles analogous to supernovae, since their large redshift range and high luminosities make them excellent candidates. The reverberation mapping (RM) method enables one to estimate the distance to the sourc... | [
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Bayesian Inference of High-density Nuclear Symmetry Energy from Radii of Canonical Neutron Stars. The radius R 1.4 of neutron stars (NSs) with a mass of 1.4 M ⊙ has been extracted consistently in many recent studies in the literature. Using representative R 1.4 data, we infer high-density nuclear symmetry energy E sym(... | [
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In the Galactic Disk, Stellar [Fe/H] and Age Predict Orbits and Precise [X/Fe]. We explore the structure of the element abundance-age-orbit distribution of the stars in the Milky Way’s low-α disk, by (re-)deriving precise [Fe/H], [X/Fe], and ages, along with orbits, for red clump stars from the APOGEE survey. There has... | [
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Fast-to-Alfvén Mode Conversion and Ambipolar Heating in Structured Media. II. Numerical Simulation. This paper studies the effectiveness of production of Alfvén waves in the solar atmosphere through the processes of mode conversion, taking into account several new effects that have not been considered before. We perfor... | [
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Cloud Atlas: Variability in and out of the Water Band in the Planetary-mass HD 203030B Points to Cloud Sedimentation in Low-gravity L Dwarfs. We use the Wide Field Camera 3 on the Hubble Space Telescope to spectrophotometrically monitor the young L7.5 companion HD 203030B. Our time series reveal photometric variability... | [
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Tidal-locking-induced Stellar Rotation Dichotomy in the Open Cluster NGC 2287?. Stars spend most of their lifetimes on the “main sequence” (MS) in the Hertzsprung-Russell diagram. The obvious double MSs seen in the equivalent color-magnitude diagrams characteristic of Milky Way open clusters (OCs) pose a fundamental ch... | [
"http://astrothesaurus.org/uat/1160",
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The Astrochemical Impact of Cosmic Rays in Protoclusters. II. CI-to-H<SUB>2</SUB> and CO-to-H<SUB>2</SUB> Conversion Factors. We utilize a modified astrochemistry code that includes cosmic-ray (CR) attenuation in situ to quantify the impact of different CR models on the CO-to-H2 and CI-to-H2 conversion factors, X CO an... | [
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Synthetic Extreme-ultraviolet Emissions Modulated by Leaky Fast Sausage Modes in Solar Active Region Loops. We study the extreme-ultraviolet (EUV) emissions modulated by leaky fast sausage modes (FSMs) in solar active region (AR) loops and examine their observational signatures via spectrometers like the EUV imaging sp... | [
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Searches for Interstellar HCCSH and H<SUB>2</SUB>CCS. A longstanding problem in astrochemistry is the inability of many current models to account for missing sulfur content. Many relatively simple species that may be good candidates to sequester sulfur have not been measured experimentally at the high spectral resoluti... | [
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The Optical Afterglow of GW170817: An Off-axis Structured Jet and Deep Constraints on a Globular Cluster Origin. We present a revised and complete optical afterglow light curve of the binary neutron star merger GW170817, enabled by deep Hubble Space Telescope (HST) F606W observations at ≈584 days post-merger, which pro... | [
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The Origin of the X-Ray Emission in Two Well-aligned Extragalactic Jets: The Case for IC/CMB. Over the past two decades, the most commonly adopted explanation for high and hard X-ray emission in resolved quasar jets has been inverse-Compton upscattering of the cosmic microwave background (IC/CMB), which requires jets t... | [
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A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension. Motivated by the current status of cosmological observations and significant tensions in the estimated values of some key parameters assuming the standard ΛCDM model, we propose a simple but radical phenomenological emergent dark energ... | [
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A Fundamental Plane for Gamma-Ray Pulsars. We show that the γ-ray pulsar observables, i.e., their total γ-ray luminosity, {L}γ , spectral cutoff energy, {ɛ }cut}, stellar surface magnetic field, B ⋆, and spin-down power \dot{{ \mathcal E }}, obey a relation of the form {L}γ =f({ɛ }cut},{B}\star ,\dot{{ \mathcal E }}), ... | [
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A Gaia-Enceladus Analog in the EAGLE Simulation: Insights into the Early Evolution of the Milky Way. We identify a simulated Milky Way analog in the EAGLE suite of cosmological hydrodynamical simulations. This galaxy not only shares similar global properties as the Milky Way, but was specifically selected because its m... | [
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Binary Mergers near a Supermassive Black Hole: Relativistic Effects in Triples. We study the general relativistic (GR) effects induced by a spinning supermassive black hole on the orbital and spin evolution of a merging black hole binary (BHB) in a hierarchical triple system. A sufficiently inclined outer orbit can exc... | [
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High-fidelity Imaging of the Inner AU Mic Debris Disk: Evidence of Differential Wind Sculpting?. We present new high-fidelity optical coronagraphic imagery of the inner ∼50 au of AU Mic’s edge-on debris disk using the BAR5 occulter of the Hubble Space Telescope Imaging Spectrograph (HST/STIS) obtained on 2018 July 26-2... | [
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"http://astrothesaurus.org/uat/994",
"http://astrothesaurus.org/uat/1629",
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Dependence of 3D Self-correlation Level Contours on the Scales in the Inertial Range of Solar Wind Turbulence. The self-correlation level contours at the 1010 cm scale reveal a 3D isotropic feature in the slow solar wind and a quasi-anisotropic feature in the fast solar wind. However, the 1010 cm scale is approximately... | [
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"http://astrothesaurus.org/uat/1534",
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Discovery of a Pulse-phase-transient Cyclotron Line in the X-Ray pulsar GRO J2058+42. We report the discovery of absorption features in the X-ray spectrum of the transient X-ray pulsar GRO J2058+42. The features are detected around ∼10, ∼20, and ∼30 keV in both NuSTAR observations carried out during the source type II ... | [
"http://astrothesaurus.org/uat/1108",
"http://astrothesaurus.org/uat/1811",
"http://astrothesaurus.org/uat/153"
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"http://astrothesaurus.org/uat/1164",
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The Pivot Energy of Solar Energetic Particles Affecting the Martian Surface Radiation Environment. Space radiation is a major risk for humans, especially on long-duration missions to outer space, e.g., a manned mission to Mars. Galactic cosmic rays contribute a predictable radiation background; the main risk is due to ... | [
"http://astrothesaurus.org/uat/1491",
"http://astrothesaurus.org/uat/2037",
"http://astrothesaurus.org/uat/1007",
"http://astrothesaurus.org/uat/1472",
"http://astrothesaurus.org/uat/2088",
"http://astrothesaurus.org/uat/329"
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"Space weather",
"Mars",
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NuSTAR Discovery of Dead Quasar Engine in Arp 187. Recent active galactic nucleus (AGN) and quasar surveys have revealed a population showing rapid AGN luminosity variability by a factor of ∼10. Here we present the most drastic AGN luminosity decline by a factor of ≳103 constrained by a NuSTAR X-ray observation of the ... | [
"http://astrothesaurus.org/uat/2035",
"http://astrothesaurus.org/uat/16"
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"http://astrothesaurus.org/uat/1569",
"http://astrothesaurus.org/uat/1671",
"http://astrothesaurus.org/uat/1696"
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