activity
20172020
most citedPolluted White Dwarfs: Mixing Regions and Diffusion Timescales

50 citations · 196 across the 6 of their papers we have counts for

collaborators

8 papers

astro-ph.SR202023 cited

Cool, Luminous, and Highly Variable Stars in the Magellanic Clouds from ASAS-SN: Implications for Thorne-Żytkow Objects and Super-Asymptotic Giant Branch Stars

Anna J. G. O'Grady, Maria R. Drout, B. J. Shappee +9

Stars with unusual properties can provide a wealth of information about rare stages of stellar evolution and exotic physics. However, determining the true nature of peculiar stars…

astro-ph.SR202050 cited

A new class of Roche lobe-filling hot subdwarf binaries

Thomas Kupfer, Evan B. Bauer, Kevin B. Burdge +30

We present the discovery of the second binary with a Roche lobe-filling hot subdwarf transferring mass to a white dwarf (WD) companion. This 56 minute binary was discovered using d…

astro-ph.SR2020

The first ultracompact Roche lobe-filling hot subdwarf binary

Thomas Kupfer, Evan B. Bauer, Thomas R. Marsh +29

We report the discovery of the first short period binary in which a hot subdwarf star (sdOB) fills its Roche lobe and started mass transfer to its companion. The object was discove…

astro-ph.SR2019

EVR-CB-001: An evolving, progenitor, white dwarf compact binary discovered with the Evryscope

Jeffrey K. Ratzloff, Brad N. Barlow, Thomas Kupfer +7

We present EVR-CB-001, the discovery of a compact binary with an extremely low mass () helium core white dwarf progenitor (pre-He WD) and an unseen low mass…

astro-ph.GA201947 cited

A new class of pulsating hot subdwarfs

Thomas Kupfer, Evan B. Bauer, Kevin B. Burdge +22

Using high-cadence observations from the Zwicky Transient Facility at low Galactic latitudes, we have discovered a new class of pulsating, hot, compact stars. We have found four ca…

astro-ph.SR2019

Remnants of Subdwarf Helium Donor Stars Ejected from Close Binaries with Thermonuclear Supernovae

Evan B. Bauer, Christopher J. White, Lars Bildsten

Some binary systems composed of a white dwarf (WD) and a hot subdwarf (sdB) helium star will make contact within the helium burning lifetime of the sdB star. The accreted helium on…