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IRAS Minor Planet Survey (IMPS) Data Set V6.0. The V6.0 version of this data set comprises the 2002 Supplemental IRAS Minor Planet Survey (SIMPS) which presents additional and revised diameters and albedos for asteroids detected by the 1983 IRAS mission. This version supersedes versions 1.0 through 5.0, which represent... | [
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TNO and Centaur Diameters, Albedos, and Densities Bundle V1.0. This data set is a compilation of published diameters, albedos, and densities for Transneptunian Objects (TNOs) and Centaurs. A total of 194 objects are listed, many with more than one entry. This version covers published values through 31 March 2018. | [
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Saturn Small Moon Shape Models Bundle V1.0. Digital shape models have been constructed from Cassini Imaging Science Subsystem (ISS) data for eleven of the small satellites of Saturn and delivered to the Planetary Data System. These satellites are: Pan, Daphnis, Atlas, Prometheus, Pandora, Epimetheus, Janus, Telesto, Ca... | [
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The Fermi Paradox and the Aurora Effect: Exo-civilization Settlement, Expansion, and Steady States. We model the settlement of the Galaxy by space-faring civilizations in order to address issues related to the Fermi Paradox. We are motivated to explore the problem in a way that avoids assumptions about the agency (i.e.... | [
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Identification of Stellar Flares Using Differential Evolution Template Optimization. We explore methods for the identification of stellar flare events in irregularly sampled data of ground-based time domain surveys. In particular, we describe a new technique for identifying flaring stars, which we have implemented in a... | [
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Untangling the Galaxy. I. Local Structure and Star Formation History of the Milky Way. Gaia DR2 provides unprecedented precision in measurements of the distance and kinematics of stars in the solar neighborhood. Through applying unsupervised machine learning on DR2's 5D data set (3D position + 2D velocity), we identify... | [
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The X-Ray-resolved Supernova Remnant S8 in the Dwarf Irregular Galaxy IC 1613. We conducted an observation of the nearby irregular galaxy IC 1613 with the Chandra X-ray Observatory using the S3 chip of the Advanced CCD Imaging Spectrometer (ACIS) with an effective exposure time of 49.9 ks. The observation primarily tar... | [
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Looking for Lurkers: Co-orbiters as SETI Observables. A recently discovered group of nearby co-orbital objects is an attractive location for extraterrestrial intelligence (ETI) to locate a probe to observe Earth while not being easily seen. These near-Earth objects provide an ideal way to watch our world from a secure ... | [
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Two Long-period Cataclysmic Variable Stars: ASASSN-14ho and V1062 Cyg. We report spectroscopy and photometry of the cataclysmic variable stars ASASSN-14ho and V1062 Cyg. Both are dwarf novae with spectra dominated by their secondary stars, which we classify approximately as K4 and M0.5, respectively. Their orbital peri... | [
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Spitzer Phase Curves of KELT-1b and the Signatures of Nightside Clouds in Thermal Phase Observations. We observed two full orbital phase curves of the transiting brown dwarf KELT-1b, at 3.6 and 4.5 μm, using the Spitzer Space Telescope. Combined with previous eclipse data from Beatty et al., we strongly detect KELT-1b... | [
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Speckle Observations and Orbits of Multiple Stars. We report results of speckle-interferometric monitoring of visual hierarchical systems using the newly commissioned instrument NN-EXPLORE Exoplanet and Stellar Speckle Imager at the 3.5 m WIYN telescope. During one year, 390 measurements of 129 resolved subsystems were... | [
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WISE J072003.20-084651.2B is a Massive T Dwarf. We present individual dynamical masses for the nearby M9.5+T5.5 binary WISE J072003.20-084651.2AB, a.k.a. Scholz’s star. Combining high-precision Canada-France-Hawaii Telescope/WIRCam photocenter astrometry and Keck adaptive optics resolved imaging, we measure the first h... | [
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Near-resonance in a System of Sub-Neptunes from TESS. We report the Transiting Exoplanet Survey Satellite detection of a multi-planet system orbiting the V = 10.9 K0 dwarf TOI-125. We find evidence for up to five planets, with varying confidence. Three transit signals with high signal-to-noise ratio correspond to sub-N... | [
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Searching for Black Hole Candidates by LAMOST and ASAS-SN. Most dynamically confirmed stellar-mass black holes (BHs) and their candidates were originally selected from X-ray outbursts. In the present work, we search for BH candidates in the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) survey using... | [
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Observation, Modern Light-curve Analysis, and 89 yr Period Study of the Short-period Algol, AE Cassiopeia. AE Cas was observed some 40 yr ago by Srivastava & Kandpal and was analyzed by Kopal’s Fourier frequency -domain technique. No further precision observations have taken place until the present study, which rep... | [
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Spectroscopic Follow-up of Discoveries from the NEOWISE Proper Motion Survey. We present low-resolution near-infrared spectra of discoveries from an all-sky proper motion search conducted using multi-epoch data from the Wide-field Infrared Survey Explorer. Using the data from NEOWISE, along with the AllWISE catalog, Sc... | [
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The Contribution of Dwarf Planets to the Origin of Jupiter Family Comets. We explore the long-term evolution of a bias-free orbital representation of the cometary nuclei (with diameters above 2 km) of the Kuiper Belt, using the so-called L7 synthetic model from CFEPS, which consists of three dynamical subpopulations: t... | [
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Constraints on the Occurrence and Distribution of 1-20 M <SUB>Jup</SUB> Companions to Stars at Separations of 5-5000 au from a Compilation of Direct Imaging Surveys. We present the first statistical analysis of exoplanet direct imaging surveys combining adaptive optics (AO) imaging at small separations with deep seeing... | [
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Hot Jupiters Are Destroyed by Tides While Their Host Stars Are on the Main Sequence. While cooler giant planets are often observed with nonzero eccentricities, the short-period circular orbits of hot Jupiters suggest that they lose orbital energy and angular momentum due to tidal interactions with their host stars. How... | [
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He II Emission from Wolf-Rayet Stars as a Tool for Measuring Dust Reddening. We calibrated a technique to measure dust attenuation in star-forming galaxies. The technique utilizes the stellar-wind lines in Wolf-Rayet stars, which are widely observed in galaxy spectra. The He II 1640 and 4686 features are recombination ... | [
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Jupiter's Composition Suggests its Core Assembled Exterior to the N<SUB>2</SUB> Snowline. Jupiter's atmosphere is enriched in C, N, S, P, Ar, Kr, and Xe with respect to solar abundances by a factor of ∼3. Gas giant envelopes are mainly enriched through the dissolution of solids in the atmosphere, and this constant enri... | [
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Predicting the Yield of Potential Venus Analogs from TESS and Their Potential for Atmospheric Characterization. The transit method is biased toward short orbital period planets that are interior to their host star’s habitable zone. These planets are particularly interesting from the perspective of exploring runaway gre... | [
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KELT-24b: A 5M <SUB>J</SUB> Planet on a 5.6 day Well-aligned Orbit around the Young V = 8.3 F-star HD 93148. We present the discovery of KELT-24 b, a massive hot Jupiter orbiting a bright (V = 8.3 mag, K = 7.2 mag) young F-star with a period of 5.6 days. The host star, KELT-24 (HD 93148), has a T eff = {6509}-49+50 K, ... | [
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Stellar Properties of KIC 8736245: An Eclipsing Binary with a Solar-type Star Leaving the Main Sequence. There is a well-known stellar parameter discrepancy for late K and M dwarfs, in that the observed radii and temperatures are often respectively larger and cooler than predicted by theory by several percent. In an on... | [
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Radial Velocity Measurements of HR 8799 b and c with Medium Resolution Spectroscopy. High-contrast medium resolution spectroscopy has been used to detect molecules such as water and carbon monoxide in the atmospheres of gas giant exoplanets. In this work, we show how it can be used to derive radial velocity (RV) measur... | [
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The Young Massive Star Cluster Westerlund 2 Observed with MUSE. II. MUSEpack—A Python Package to Analyze the Kinematics of Young Star Clusters. We mapped the Galactic young massive star cluster Westerlund 2 with the integral field spectrograph MUSE (spatial resolution: 0.2 arcsec px-1, spectral resolution: ∆λ = 1.25 Å,... | [
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The Role of Cluster Mass in the Multiple Populations of Galactic and Extragalactic Globular Clusters. Studies based on Hubble Space Telescope (HST) photometry in F275W, F336W, and F438W have shown that the incidence and complexity of multiple populations (MPs) in globular clusters (GCs) depend on cluster mass. This res... | [
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Compositional Constraints for Lucy Mission Trojan Asteroids via Near-infrared Spectroscopy. We report near-infrared (0.7-2.5 μm) reflectance spectra for each of the six target asteroids of the forthcoming NASA Discovery-class mission Lucy. Five Jupiter Trojans (the binary (617) Patroclus system, (3548) Eurybates, (2190... | [
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Revisiting the Advanced Thermal Physical Model: New Perspectives on Thermophysical Characteristics of (341843) 2008 EV5 from Four-band WISE Data with the Sunlight-reflection Model. In this paper, we investigate thermophysical characteristics of near-Earth asteroid (341843) 2008 EV5, based on our improved advanced therm... | [
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Kojima-1Lb Is a Mildly Cold Neptune around the Brightest Microlensing Host Star. We report the analysis of additional multiband photometry and spectroscopy and new adaptive optics (AO) imaging of the nearby planetary microlensing event TCP J05074264+2447555 (Kojima-1), which was discovered toward the Galactic anticente... | [
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Model of the Search for Extraterrestrial Intelligence with Coronagraphic Imaging. We present modeled detection limits of the Gemini Planet Imager (GPI) and the Wide-Field Infrared Space Telescope (WFIRST) to an optical and infrared laser which could be used by an extraterrestrial civilization to signal their presence. ... | [
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First Detection of CS Masers around a High-mass Young Stellar Object, W51 e2e. We report the discovery of maser emission in the two lowest rotational transitions of CS toward the high-mass protostar W51 e2e with the Atacama Large Millimeter/submillimeter Array and the Jansky Very Large Array. The masers from CS J = 1-0... | [
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In the Presence of a Wrecking Ball: Orbital Stability in the HR 5183 System. Discoveries of exoplanets using the radial velocity method are progressively reaching out to increasingly longer orbital periods as the duration of surveys continues to climb. The improving sensitivity to potential Jupiter analogs is revealing... | [
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Hubble Space Telescope Flux Calibration. I. STIS and CALSPEC. The precision of absolute flux measurements is quantified for the Space Telescope Imaging Spectrograph (STIS), which is the most important contributor to the CALSPEC standards. With our goal of 1% absolute accuracy, the documentation of the Hubble Space Tele... | [
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OGLE-2015-BLG-1649Lb: A Gas Giant Planet around a Low-mass Dwarf. We report the discovery of an exoplanet from the analysis of the gravitational microlensing event OGLE-2015-BLG-1649 that challenges the core accretion model of planet formation and appears to support the disk instability model. The planet/host-star mass... | [
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CCD Measurements of Double and Multiple Stars at ASV and NAO Rozhen in 2017 and 2018. We give the results of CCD observations for 789 double or multiple stars obtained during 2017 and 2018. These observations were carried out at both the Serbian Astronomical Station on the mountain of Vidojevica (ASV) and the Bulgarian... | [
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Investigating Trends in Atmospheric Compositions of Cool Gas Giant Planets Using Spitzer Secondary Eclipses. We present new 3.6 and 4.5 μm secondary eclipse measurements for five cool (T ≲ 1000 K) transiting gas giant planets: HAT-P-15b, HAT-P-17b, HAT-P-18b, HAT-P-26b, and WASP-69b. We detect eclipses in at least one ... | [
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Visual Orbits of Spectroscopic Binaries with the CHARA Array. II. The Eclipsing Binary HD 185912. We present the visual orbit of the double-lined eclipsing binary, HD 185912, from long baseline interferometry with the CHARA Array. We also obtain echelle spectra from the Apache Point observatory to update the spectrosco... | [
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Investigating the Temperature Distribution of Diatomic Carbon in Comets Using the Swan Bands. We present high spectral resolution observations of comets 122P/de Vico and 153P/Ikeya-Zhang obtained with the Tull Coudé spectrograph on the 2.7 m Harlan J. Smith telescope of McDonald Observatory. We used these data to study... | [
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Spectroscopic Orbits of Subsystems in Multiple Stars. VI.. Thirteen spectroscopic orbits of late-type stars are determined from the high-resolution spectra taken with the CHIRON echelle spectrometer at the 1.5 m Cerro Tololo Inter-American Observatory telescope. Most (HIP 14194B, 40523A, 41171A, 51578A, 57572B, 59426A,... | [
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Kinematics of the Palomar 5 Stellar Stream from RR Lyrae Stars. Thin stellar streams, formed from the tidal disruption of globular clusters, are important gravitational tools, sensitive to both global and small-scale properties of dark matter. The Palomar 5 stellar stream (Pal 5) is an exemplar stream within the Milky ... | [
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MOA-bin-29b: A Microlensing Gas-giant Planet Orbiting a Low-mass Host Star. We report the discovery of a gas-giant planet orbiting a low-mass host star in the microlensing event MOA-bin-29 that occurred in 2006. We find five degenerate solutions with the planet/host-star mass ratio of q ∼ 10-2. The Einstein radius cros... | [
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"http://astrothesaurus.org/uat/1295",
"http://astrothesaurus.org/uat/1634",
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Detection of a Low-mass Stellar Companion to the Accelerating A2IV Star HR 1645. The ∼500 Myr A2IV star HR 1645 has one of the most significant low-amplitude accelerations of nearby early-type stars measured from a comparison of the Hipparcos and Gaia astrometric catalogs. This signal is consistent with either a stella... | [
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HyDRA-H: Simultaneous Hybrid Retrieval of Exoplanetary Emission Spectra. High-resolution Doppler spectroscopy has been used to detect several chemical species in exoplanetary atmospheres. Such detections have traditionally relied on cross correlation of observed spectra against spectral model templates, an approach tha... | [
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Ultraviolet Imaging Telescope View of Dwarf Irregular Galaxy IC 2574: Is the Star Formation Triggered Due to Expanding H I Shells?. Star-forming dwarf galaxies in the local volume are diverse and ideal test beds to understand the details of star formation in a variety of environments. Here we present a deep far-UV (FUV... | [
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IRAS 09002-4732: A Laboratory for the Formation of Rich Stellar Clusters. IRAS 09002-4732 is a poorly studied embedded cluster of stars in the Vela Molecular Ridge at a distance of 1.7 kpc. Deep observations with the Chandra X-ray Observatory, combined with existing optical and infrared surveys, produce a catalog of 44... | [
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New Constraint on the Atmosphere of (50000) Quaoar from a Stellar Occultation. We report observations of a stellar occultation by the classical Kuiper Belt object (50000) Quaoar that occurred on 2019 June 28. A single-chord high-cadence (2 Hz) photometry data set was obtained with the Tomo-e Gozen CMOS camera mounted o... | [
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Image Flux Ratios of Gravitationally Lensed HS 0810+2554 with High-resolution Infrared Imaging. We report near simultaneous imaging using LMIRCam on the LBTI of the quadruply imaged lensed quasar HS 0810+2554 at wavelengths of 2.16, 3.7, and 4.78 μm with a full width at half maximum spatial resolution of 0.″13, 0.″12, ... | [
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An Integrable Model for the Dynamics of Planetary Mean-motion Resonances. I consider the dynamics of mean-motion resonances (MMRs) between pairs of coplanar planets and derive a new integrable Hamiltonian model for the planets’ resonant motion. The new model generalizes integrable Hamiltonians previously derived for fi... | [
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Do Metal-rich Stars Make Metal-rich Planets? New Insights on Giant Planet Formation from Host Star Abundances. The relationship between the compositions of giant planets and their host stars is of fundamental interest in understanding planet formation. The solar system giant planets are enhanced above solar composition... | [
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Gaia 19ajj: A Young Star Brightening Due to Enhanced Accretion and Reduced Extinction. We report on the source Gaia 19ajj, identifying it as a young star associated with a little-studied star-forming region seen along a complex line of sight through the Gum Nebula. The optical lightcurve recently recorded by Gaia exhib... | [
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The New EXor Outburst of ESO-Hα 99 Observed by Gaia ATLAS and TESS. We report photometry and spectroscopy of the outburst of the young stellar object ESO-Hα99. The outburst was first noticed in Gaia alert Gaia18dvc and later by the Asteroid Terrestrial-impact Last Alert System (ATLAS). We have established the outburst ... | [
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Compositions of Planetary Debris around Dusty White Dwarfs. The photospheres of some white dwarfs (WDs) are “polluted” by accretion of material from their surrounding planetary debris. WDs with dust disks are often heavily polluted and high-resolution spectroscopic observations of these systems can be used to infer the... | [
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A Search for Multiplanet Systems with TESS Using a Bayesian N-body Retrieval and Machine Learning. Transiting exoplanets in multiplanet systems exhibit non-Keplerian orbits as a result of the gravitational influence from companions, which can cause the times and durations of transits to vary. The amplitude and periodic... | [
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A Hubble PanCET Study of HAT-P-11b: A Cloudy Neptune with a Low Atmospheric Metallicity. We present the first comprehensive look at the 0.35-5 μm transmission spectrum of the warm (∼800 K) Neptune HAT-P-11b derived from 13 individual transits observed using the Hubble and Spitzer Space Telescopes. Along with the previo... | [
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Accretion Kinematics in the T Tauri Binary TWA 3A: Evidence for Preferential Accretion onto the TWA 3A Primary. We present time-series, high-resolution optical spectroscopy of the eccentric T Tauri binary TWA 3A. Our analysis focuses on variability in the strength and structure of the accretion-tracing emission lines H... | [
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Solar Neighborhood Kinematics from Gaia -LAMOST Dwarf Stars. We use high-precision kinematic data from Gaia data release 2 (DR2) and spectroscopic data from Large Sky Area Multi-Object Fibre Spectroscopic Telescope (LAMOST) data release 5 (DR5) to explore the kinematics of solar neighborhood dwarf stars in the northern... | [
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Asteroseismology of the Multiplanet System K2-93. We revisit the analysis of the bright multiplanet system K2-93, discovered with data taken by the K2 mission. This system contains five identified planets ranging in size from sub-Neptune to Jupiter size. The K2 data available at the discovery of the system only showed ... | [
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Super Metal-rich Stars in the LAMOST Survey: A Test on Radial Migration. Super metal-rich stars with [Fe/H] > 0.4 are selected from LAMOST DR6, and two groups, the blue and the red, are found in the T eff versus logg diagram with a temperature gap between them. In combination with Gaia DR2, stellar positions, veloci... | [
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Compact Survey Telescope with a Diameter of 3.6 m. An optical layout of a corrected Cassegrain telescope with an aperture of 3.6 m (f/3.0) and a 2.°5 field of view is proposed. The primary and secondary mirrors are standard hyperboloids; all five corrector lenses are made of fused silica and have spherical surfaces. Th... | [
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A Reanalysis of the UVES M Dwarf Planet Search Program. The UVES (Ultraviolet and Visible Spectrometer) M Dwarf Planet Search program surveyed 40 M dwarfs and 1 M giant from 2000 through 2007 March. Two of the M dwarfs were double-lined spectroscopic binaries. The 38 single-lined M dwarfs in this survey are among the n... | [
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Upper Limits for Emissions in the Coma of Comet 67P/Churyumov-Gerasimenko near Perihelion as Measured by Rosetta’s Alice Far-UV Spectrograph. The Alice far-UV imaging spectrograph (700-2050 Å) acquired over 70,000 spectral images during Rosetta’s 2 yr escort mission, including over 20,000 in the months surrounding peri... | [
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Low-frequency Radio Absorption in Tycho’s Supernova Remnant. Tycho’s supernova remnant (SNR) is the remnant of the SN Ia explosion SN1572. In this work we present new low-frequency radio observations with the LOw Frequency ARray (LOFAR) Low-band and High-band Antennae, centered at 58 MHz and 143 MHz, and with an angula... | [
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Quantifying the Evolution of Molecular Production Rates of Comet 21P/Giacobini-Zinner with iSHELL/NASA-IRTF. This paper presents results from our molecular characterization of comet 21P/Giacobini-Zinner during its 2018 apparition. We followed the comet during four observing runs, for a total of eight nights. The high-r... | [
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Physical Characterization of the 2017 December Outburst of the Centaur 174P/Echeclus. The Centaurs are the small solar system bodies intermediate between the active inner solar system Jupiter family comets and their inactive progenitors in the trans-Neptunian region. Among the fraction of Centaurs which show comet-like... | [
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New Insights into Interstellar Object 1I/2017 U1 (‘Oumuamua) from SOHO/STEREO Nondetections. Object 1I/2017 U1 (‘Oumuamua) is the first interstellar small body ever discovered in the solar system. By the time of discovery, it had already passed perihelion. To investigate the behavior of ‘Oumuamua around perihelion, we ... | [
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Avocado: Photometric Classification of Astronomical Transients with Gaussian Process Augmentation. Upcoming astronomical surveys such as the Large Synoptic Survey Telescope (LSST) will rely on photometric classification to identify the majority of the transients and variables that they discover. We present a set of tec... | [
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Improved Analysis of Clarke Exobelt Detectability. We analyze the potential transit light curve effects due to a Clarke belt of satellites around an exoplanet. Building on code and analysis from Korpela et al., we refine the transit analysis of Socas-Navarro by incorporating limb-darkening and taking an observer-center... | [
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Analysis of HST WFPC2 Observations of Centaur 29P/Schwassmann-Wachmann 1 while in Outburst to Place Constraints on the Nucleus’ Rotation State. We present analysis of Hubble Space Telescope observations of Centaur 29P/Schwassmann-Wachmann 1 (SW1) while in outburst to characterize the outburst coma and place constraints... | [
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Optical Reddening, Integrated H I Optical Depth, and Total Hydrogen Column Density. Despite the vastly different angular scales on which they are measured, the integrated λ21 cm H I optical depth measured interferometrically, {{{\Upsilon }}}{{H}{{I}}}, is a good proxy for the optical reddening derived from IR dust emis... | [
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Graze-and-merge Collisions under External Perturbers. Graze-and-merge collisions are common multi-step mergers occurring in low-velocity, off-axis impacts between similar-sized planetary bodies. The first impact happens at somewhat faster than the mutual escape velocity; for typical impact angles this does not result i... | [
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Hot Hydrogen Climates Near the Inner Edge of the Habitable Zone. Young terrestrial planets can capture or outgas hydrogen-rich atmospheres with tens to hundreds of bars of H2, which persist for 100 Myr or longer. Although the earliest habitable conditions on Earth and terrestrial exoplanets could thus arise while the a... | [
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Most Black Holes Are Born Very Slowly Rotating. The age of gravitational-wave astronomy has begun, and black hole (BH) mergers detected by the Laser Interferometer Gravitational-Wave Observatory (LIGO) are providing novel constraints on massive star evolution. A major uncertainty in stellar theory is the angular moment... | [
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Single-spacecraft Identification of Flux Tubes and Current Sheets in the Solar Wind. A novel technique is presented for describing and visualizing the local topology of the magnetic field using single-spacecraft data in the solar wind. The approach merges two established techniques: the Grad-Shafranov (GS) reconstructi... | [
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Constraining the Solar System's Debris Disk with In Situ New Horizons Measurements from the Edgeworth-Kuiper Belt. The solar system currently possesses two remnant debris disks leftover from the planetary formation era in the form of the asteroid belt and the Edgeworth-Kuiper Belt (EKB). Similar to other stellar system... | [
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Compact Object Binary Mergers Driven By Cluster Tides: A New Channel for LIGO/Virgo Gravitational-wave Events. The detections of gravitational waves (GWs) produced in mergers of binary black holes (BHs) and neutron stars (NSs) by LIGO/Virgo have stimulated interest in the origin of the progenitor binaries. Dense stella... | [
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Smoothing of MHD Shocks in Mode Conversion. Shock waves are simulated passing through the Alfvén-acoustic equipartition layer in a stratified isothermal magneto-atmosphere. The recent ray-theoretic calculations of Núñez predicted smoothing of the shock through this layer, causing both the fast and slow components to em... | [
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Reconnection Front Associated with Asymmetric Magnetic Reconnection: Particle-in-cell Simulations. Reconnection front (RF) has frequently been observed in the magnetotail and is well known as the dipolarization front in the near-Earth tail. Whether the RF exists in reconnection with distinct plasma/field properties acr... | [
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Searches after Gravitational Waves Using ARizona Observatories (SAGUARO): System Overview and First Results from Advanced LIGO/Virgo’s Third Observing Run. We present Searches After Gravitational-waves Using ARizona Observatories (SAGUARO), a comprehensive effort dedicated to the discovery and characterization of optic... | [
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The Role of Upper Hybrid Waves in the Magnetotail Reconnection Electron Diffusion Region. Plasma waves are believed to play an important role during magnetic reconnection. However, the specific role of upper hybrid (UH) waves in the electron diffusion region (EDR) remains elusive, owing to the absence of high-resolutio... | [
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Electron Mirror-mode Structure: Magnetospheric Multiscale Observations. The small-scale mirror mode excited by electron dynamics is a fundamental physical process, attracting research interest in space, laboratory, and astrophysical plasma physics over the past half century. However, the investigations of this process ... | [
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Type I Outbursts in Low-eccentricity Be/X-Ray Binaries. Type I outbursts in Be/X-ray binaries are usually associated with the eccentricity of the binary orbit. The neutron star accretes gas from the outer parts of the decretion disk around the Be star at each periastron passage. However, this mechanism cannot explain t... | [
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Detection of Propadiene on Titan. The atmosphere of Titan, the largest moon of Saturn, is rich in organic molecules, and it has been suggested that the moon may serve as an analog for the pre-biotic Earth due to its highly reducing chemistry and existence of global hazes. Photochemical models of Titan have predicted th... | [
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The MOSDEF Survey: Sulfur Emission-line Ratios Provide New Insights into Evolving Interstellar Medium Conditions at High Redshift. We present results on the emission-line properties of 1.3 ≤ z ≤ 2.7 galaxies drawn from the complete the MOSFIRE Deep Evolution Field (MOSDEF) survey. Specifically, we use observations of t... | [
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On the Fast Solar Wind Heating and Acceleration Processes: A Statistical Study Based on the UVCS Survey Data. The UltraViolet Coronagraph Spectrometer (UVCS) on board the SOlar and Heliospheric Observatory has almost continuously observed, throughout the whole solar cycle 23, the UV solar corona. This work addresses th... | [
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Viewing Angle Constraints on S190425z and S190426c and the Joint Gravitational-wave/Gamma-Ray Detection Fractions for Binary Neutron Star Mergers. The Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo scientific collaboration (LVC) detected two binary neutron star (BNS) merger candidates, S190425z an... | [
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Prospects for Gravitational Wave Measurement of ZTF J1539+5027. The short-period eclipsing binary ZTF J1539+5027 discovered by Burdge et al. will be a strong gravitational-wave source for the Laser Interferometer Space Antenna (LISA). We study how well LISA will constrain the parameters of this system by analyzing simu... | [
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The Kennicutt-Schmidt Law and Gas Scale Height in Luminous and Ultraluminous Infrared Galaxies. A new analysis of high-resolution data from the Atacama Large Millimeter/submillimeter Array for five luminous or ultraluminous infrared galaxies gives a slope for the Kennicutt-Schmidt (KS) relation equal to {1.74}-0.07+0.0... | [
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X-Ray and Gamma-Ray Emission from Core-collapse Supernovae: Comparison of Three-dimensional Neutrino-driven Explosions with SN 1987A. During the first few hundred days after the explosion, core-collapse supernovae (SNe) emit down-scattered X-rays and gamma-rays originating from radioactive line emissions, primarily fro... | [
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Temperature Fluctuation at the Sun and Large-scale Electric Field in Solar Wind: A Challenge for the Parker Solar Probe Mission. Velocity distributions of particles are key elements in the study of solar wind. The physical mechanisms that regulate their many features are a matter of debate. The present work addresses t... | [
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The Lanthanide Fraction Distribution in Metal-poor Stars: A Test of Neutron Star Mergers as the Dominant r-process Site. Multimessenger observations of the neutron star merger GW170817 and its kilonova proved that neutron star mergers can synthesize large quantities of r-process elements. If neutron star mergers in fac... | [
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Differentiation of Enceladus and Retention of a Porous Core. The Cassini mission revealed gas plumes associated with surface features called “tiger stripes” at the south pole of Saturn’s moon Enceladus. The composition of plume particles and local cryovolcanism suggested as a possible cause for the activity are typical... | [
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Understanding Uniturbulence: Self-cascade of MHD Waves in the Presence of Inhomogeneities. It is widely accepted in the MHD turbulence community that the nonlinear cascade of wave energy requires counterpropagating Alfvénic wave packets, along some mean magnetic field. This fact is an obvious outcome of the MHD equatio... | [
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In Situ Measurements of the Variable Slow Solar Wind near Sector Boundaries. The release of density structures at the tip of the coronal helmet streamers, likely as a consequence of magnetic reconnection, contributes to the mass flux of the slow solar wind (SSW). In situ measurements in the vicinity of the heliospheric... | [
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Galactic Cosmic Rays Modulation in the Vicinity of Corotating Interaction Regions: Observations During the Last Two Solar Minima. Corotating interaction regions (CIRs) are responsible for short-term recurrent cosmic-ray modulation, prominent near solar minima. Using the OMNI data sets for two periods of low solar activ... | [
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Particle Acceleration and Heating in Regions of Magnetic Flux Emergence. The interaction between emerging and pre-existing magnetic fields in the solar atmosphere can trigger several dynamic phenomena, such as eruptions and jets. A key element during this interaction is the formation of large-scale current sheets, and ... | [
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Density Conversion between 1D and 3D Stellar Models with <SUP>1D</SUP>MESA2HYDRO<SUP>3D</SUP>. We present 1DMESA2HYDRO3D, an open-source, Python-based software tool that provides an accessible means of generating physically motivated initial conditions (ICs) for hydrodynamical simulations from 1D stellar structure mode... | [
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New Star Observations with NuSTAR: Flares from Young Stellar Objects in the ρ Ophiuchi Cloud Complex in Hard X-Rays. We study the structure and dynamics of extreme flaring events on young stellar objects (YSOs) observed in hard X-rays by the Nuclear Spectroscopic Telescope Array (NuSTAR). During 2015 and 2016, NuSTAR m... | [
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"http://astrothesaurus.org/uat/1290",
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Galactic Gas Flows from Halo to Disk: Tomography and Kinematics at the Milky Way’s Disk-Halo Interface. We present a novel absorption-line survey using 54 blue horizontal branch stars in the Milky Way halo as background sources for detecting gas flows at the disk-halo interface. Distance measurements to high-latitude (... | [
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"http://astrothesaurus.org/uat/602",
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Mimetic DBI Inflation in Confrontation with Planck2018 Data. We study mimetic gravity in the presence of a Dirac-Born-Infeld (DBI)-like term, which is a non-canonical setup of the scalar field’s derivatives. We consider two general cases with varying and constant sound speeds and construct the potentials for both the D... | [
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"http://astrothesaurus.org/uat/337",
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