output
19912026
Showing 2019 · astro-ph.SRShow all

26 papers · 2 filters

astro-ph.SR2019★ 43 cited

A Catalog of M-dwarf Flares with ASAS-SN

Romy Rodríguez Martínez, Laura A. Lopez, Benjamin J. Shappee +5

We analyzed the light curves of 1376 early-to-late, nearby M dwarfs to search for white-light flares using photometry from the All-Sky Automated Survey for Supernovae (ASAS-SN). We…

astro-ph.SR2019★ 10 cited

Imaging the 44 AU Kuiper Belt-analogue debris ring around HD 141569A with GPI polarimetry

J. S. Bruzzone, S. Metchev, G. Duchene +53

We present the first polarimetric detection of the inner disk component around the pre-main sequence B9.5 star HD 141569A. Gemini Planet Imager H-band (1.65 micron) polarimetric di…

astro-ph.SR2019★ 8 cited

Discovery of a Rare Late-Type, Low-Mass Wolf-Rayet Star in the LMC

Bruce Margon, Catherine Manea, Robert Williams +4

We report the serendipitous discovery of an object, UVQS J060819.93-715737.4, with a spectrum dominated by extremely intense, narrow C II emission lines. The spectrum is similar to…

astro-ph.SR2019★ 44 cited

Common Envelope Wind Tunnel: The Effects of Binary Mass Ratio and Implications for the Accretion-Driven Growth of LIGO Binary Black Holes

Soumi De, Morgan MacLeod, Rosa Wallace Everson +3

We present three-dimensional local hydrodynamic simulations of flows around objects embedded within stellar envelopes using a "wind tunnel" formalism. Our simulations model the com…

astro-ph.SR2019★ 6 cited

Detection of a low-mass stellar companion to the accelerating A2IV star HR 1645

Robert J. De Rosa, Eric L. Nielsen, Julien Rameau +50

The \, 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 {\it Hipparcos} and {…

astro-ph.SR2019★ 42 cited

Evolutionary models for R Coronae Borealis stars

Josiah Schwab

We use Modules for Experiments in Stellar Astrophysics (MESA) to construct stellar evolution models that reach a hydrogen-deficient, carbon-rich giant phase like the R Coronae Bore…

astro-ph.SR2019★ 2 cited

Imaging Polarimetry of the 2017 Solar Eclipse with the RIT Polarization Imaging Camera

Dmitry Vorobiev, Zoran Ninkov, Lee Bernard +1

In the last decade, imaging polarimeters based on micropolarizer arrays have been developed for use in terrestrial remote sensing and metrology applications. Micropolarizer-based s…

astro-ph.SR2019★ 12 cited

New Spatially Resolved Imaging of the SR 21 Transition Disk and Constraints on the Small-Grain Disk Geometry

Steph Sallum, Andy Skemer, Josh Eisner +9

We present new 0.6 - 4 m 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…

astro-ph.SR2019★ 79 cited

The Effect of Star--Disk Interactions on Highly Eccentric Stellar Orbits in Active Galactic Nuclei: A Disk Loss Cone and Implications for Stellar Tidal Disruption Events

Morgan MacLeod, Douglas N. C. Lin

Galactic center black holes appear to be nearly universally surrounded by dense stellar clusters. When these black holes go through an active accretion phase, the multiple componen…

astro-ph.SR2019★ 43 cited

TOI-503: The first known brown dwarf-Am star binary from the TESS mission

Ján Šubjak, Rishikesh Sharma, Theron W. Carmichael +76

We report the discovery of an intermediate-mass transiting brown dwarf, TOI-503b, from the TESS mission. TOI-503b is the first brown dwarf discovered by TESS and orbits a metallic-…

astro-ph.SR2019★ 17 cited

A 9-Hr CV With One Outburst in 4 Years of Kepler Data

Zhifei Yu, John Thorstensen, Saul Rappaport +11

During a visual search through the Kepler main-field lightcurves, we have discovered a cataclysmic variable (CV) that experienced only a single 4-day long outburst over four years,…

astro-ph.SR2019★ 28 cited

A Dramatic Decrease in Carbon Star Formation in M31

M. L. Boyer, B. F. Williams, B. Aringer +8

We analyze resolved stellar near-infrared photometry of 21 HST fields in M31 to constrain the impact of metallicity on the formation of carbon stars. Observations of nearby galaxie…

astro-ph.SR2019★ 20 cited

The interaction between shear and fingering (thermohaline) convection

P. Garaud, A. Kumar, J. Sridhar

Fingering convection is a turbulent mixing process that can occur in stellar radiative regions whenever the mean molecular weight increases with radius. In some cases, it can have…

astro-ph.SR2019★ 16 cited

Discovery of a White Dwarf Companion to HD 159062

Lea A. Hirsch, David R. Ciardi, Andrew W. Howard +11

We report on the discovery of a white dwarf companion to the nearby late G dwarf star, HD 159062. The companion is detected in 14 years of precise radial velocity (RV) data, and in…

astro-ph.SR2019★ 6 cited

High Spatial Resolution Thermal-Infrared Spectroscopy with ALES: Resolved Spectra of the Benchmark Brown Dwarf Binary HD 130948BC

Zackery W. Briesemeister, Andrew J. Skemer, Jordan M. Stone +6

We present 2.9-4.1 micron integral field spectroscopy of the L4+L4 brown dwarf binary HD 130948BC, obtained with the Arizona Lenslets for Exoplanet Spectroscopy (ALES) mode of the…

astro-ph.SR2019★ 22 cited

Direct measurement of stellar angular diameters by the VERITAS Cherenkov Telescopes

W. Benbow, R. Bird, A. Brill +54

The angular size of a star is a critical factor in determining its basic properties. Direct measurement of stellar angular diameters is difficult: at interstellar distances stars a…

astro-ph.SR2019★ 5 cited

Carbon Abundance Inhomogeneities and Deep Mixing Rates in Galactic Globular Clusters

Jeffrey M. Gerber, Michael M. Briley, Graeme H. Smith

Among stars in Galactic globular clusters the carbon abundance tends to decrease with increasing luminosity on the upper red giant branch, particularly within the lowest metallicit…

astro-ph.SR2019★ 31 cited

Discovery of an intermediate-luminosity red transient in M51 and its likely dust-obscured, infrared-variable progenitor

Jacob E. Jencson, Scott M. Adams, Howard E. Bond +49

We present the discovery of an optical transient (OT) in Messier 51, designated M51 OT2019-1 (also ZTF19aadyppr, AT 2019abn, ATLAS19bzl), by the Zwicky Transient Facility (ZTF). Th…

astro-ph.SR2019★ 44 cited

Brown dwarf census with the Dark Energy Survey year 3 data and the thin disk scale height of early L types

A. Carnero Rosell, B. Santiago, M. dal Ponte +44

In this paper we present a catalogue of 11,745 brown dwarfs with spectral types ranging from L0 to T9, photometrically classified using data from the Dark Energy Survey (DES) year…

astro-ph.SR2019★ 39 cited

Cloud Atlas: Rotational Spectral Modulations and potential Sulfide Clouds in the Planetary-mass, Late T-type Companion Ross 458C

Elena Manjavacas, Daniel Apai, Ben W. P. Lew +11

Measurements of photometric variability at different wavelengths provide insights into the vertical cloud structure of brown dwarfs and planetary-mass objects. In seven Hubble Spac…

astro-ph.SR2019

Astro2020 Science White Paper: High-Resolution Spectroscopic Surveys of Ultracool Dwarf Stars & Brown Dwarfs

Adam Burgasser, Daniel Apai, Daniella Bardalez Gagliuffi +10

High resolution spectroscopy of the lowest-mass stars and brown dwarfs reveals their origins, multiplicity, compositions and physical properties, with implications for the star for…

astro-ph.SR2019★ 12 cited

Hubble Space Telescope photometry of multiple stellar populations in the inner parts of NGC 2419

S. S. Larsen, H. Baumgardt, N. Bastian +2

We present new deep imaging of the central regions of the remote globular cluster NGC 2419, obtained with the F343N and F336W filters of HST/WFC3. The new data are combined with ar…

astro-ph.SR2019★ 30 cited

A Novel Approach to Constrain Rotational Mixing & Convective-Core Overshoot in Stars Using the Initial-Final Mass Relation

Jeffrey D. Cummings, Jason S. Kalirai, Jieun Choi +3

The semi-empirical initial-final mass relation (IFMR) connects spectroscopically analyzed white dwarfs in star clusters to the initial masses of the stars that formed them. Most cu…

astro-ph.SR2019★ 22 cited

Unusual Isotopic Abundances in a Fully-Convective Stellar Binary

I. J. M. Crossfield, J. D. Lothringer, B. Flores +6

Low-mass M dwarfs represent the most common outcome of star formation, but their complex emergent spectra hinder detailed studies of their composition and initial formation. The me…