activity
20182021
most citedA hot subdwarf-white dwarf super-Chandrasekhar candidate supernova Ia progenitor

66 citations · 153 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.SR202166 cited

A hot subdwarf-white dwarf super-Chandrasekhar candidate supernova Ia progenitor

Ingrid Pelisoli, P. Neunteufel, S. Geier +8

Supernova Ia are bright explosive events that can be used to estimate cosmological distances, allowing us to study the expansion of the Universe. They are understood to result from…

astro-ph.SR202037 cited

A quantitative in-depth analysis of the prototype sdB+BD system SDSS J08205+0008 revisited in the Gaia era

V. Schaffenroth, S. L. Casewell, D. Schneider +8

Subdwarf B stars are core-helium burning stars located on the extreme horizontal branch. Extensive mass loss on the red giant branch is necessary to form them. It has been proposed…

astro-ph.SR2020

EVR-CB-004: An Inflated Hot Subdwarf O star + Unseen WD Companion in a Compact Binary Discovered with the Evryscope

Jeffrey K. Ratzloff, Thomas Kupfer, Brad N. Barlow +10

We present the discovery of EVR-CB-004, a close binary with a remnant stellar core and an unseen white dwarf companion. The analysis in this work reveals the primary is potentially…

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.SR2018

NLTE spectroscopic analysis of the He anomaly in subluminous B-type stars

D. Schneider, A. Irrgang, U. Heber +2

Several B-type main-sequence stars show chemical peculiarities. A particularly striking class are the He stars, which exhibit a remarkable enrichment of He with respect to…

astro-ph.SR2018

The MUCHFUSS photometric campaign

V. Schaffenroth, S. Geier, U. Heber +4

Hot subdwarfs (sdO/Bs) are the helium-burning cores of red giants, which lost almost all of their hydrogen envelopes. This mass loss is often triggered by common envelope interacti…