output
20022026
most citedA Catalog of Quasar Properties from SDSS DR7

1.5k citations

Showing 2021 · astro-ph.SRShow all

10 papers · 2 filters

astro-ph.SR2021★ 6 cited

Velocities of an Erupting Filament

Shuo Wang, Jack M. Jenkins, Karin Muglach +5

Solar filaments exist as stable structures for extended periods of time before many of them form the core of a CME. We examine the properties of an erupting filament on 2017 May 29…

astro-ph.SR2021★ 20 cited

Outbursts and stellar properties of the classical Be star HD 6226

Noel D. Richardson, Olivier Thizy, Jon E. Bjorkman +58

The bright and understudied classical Be star HD 6226 has exhibited multiple outbursts in the last several years during which the star grew a viscous decretion disk. We analyze 659…

astro-ph.SR2021★ 1 cited

Double-lined spectroscopic binaries in the APOGEE DR16 and DR17 data

Marina Kounkel, Kevin R. Covey, Keivan G. Stassun +25

APOGEE spectra offer 1 km s precision in the measurement of stellar radial velocities (RVs). This holds even when multiple stars are captured in the same spectrum,…

astro-ph.SR2021★ 5 cited

Symbiotic Stars in the APOGEE Survey: The Case of LIN 358 and SMC N73 (LIN 445a)

Jasmin E. Washington, Hannah M. Lewis, Borja Anguiano +9

LIN 358 and SMC N73 are two symbiotic binaries in the halo of the Small Magellanic Cloud, each composed of a hot white dwarf accreting from a cool giant companion. In this work, we…

astro-ph.SR2021★ 3 cited

The Sonora Brown Dwarf Atmosphere and Evolution Models I. Model Description and Application to Cloudless Atmospheres in Rainout Chemical Equilibrium

Mark S. Marley, Didier Saumon, Channon Visscher +8

We present a new generation of substellar atmosphere and evolution models, appropriate for application to studies of L, T, and Y-type brown dwarfs and self-luminous extrasolar plan…

astro-ph.SR2021★ 22 cited

Quasi-periodic oscillations in the TESS light curve of TX Col, a diskless intermediate polar on the precipice of forming an accretion disk

Colin Littlefield, Simone Scaringi, Peter Garnavich +4

One of the fundamental properties of an intermediate polar is the dynamical nature of the accretion flow as it encounters the white dwarf's magnetosphere. Many works have presumed…