activity
20112026
most citedHot subdwarf binaries from the MUCHFUSS project - Analysis of 12 new systems and a study of the short-period binary population

121 citations · 1.2k across the 53 of their papers we have counts for

collaborators
Showing 2020Show all

6 papers · 1 filter

astro-ph.SR2020★ 37 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★ 10 cited

EPIC 216747137: a new HW Vir eclipsing binary with a massive sdOB primary and a low-mass M-dwarf companion

R. Silvotti, V. Schaffenroth, U. Heber +8

EPIC 216747137 is a new HW~Virginis system discovered by the Kepler spacecraft during its K2 "second life". Like the other HW Vir systems, EPIC 216747137 is a post-common-envelope…

astro-ph.SR2020★ 11 cited

An extremely hot white dwarf with a rapidly rotating K-type subgiant companion: UCAC2 46706450

Klaus Werner, Nicole Reindl, Lisa Löbling +5

UCAC2 46706450 is a late-type star with an ultraviolet (UV) excess. It was considered a candidate to establish a sample of FGK stars with white dwarf (WD) companions that can be us…

astro-ph.SR2020★ 63 cited

Alone but not lonely: Observational evidence that binary interaction is always required to form hot subdwarf stars

Ingrid Pelisoli, Joris Vos, Stephan Geier +2

Hot subdwarfs are core-helium burning stars that show lower masses and higher temperatures than canonical horizontal branch stars. They are believed to be formed when a red giant s…

astro-ph.SR2020★ 47 cited

Formation of sdB-stars via common envelope ejection by substellar companions

M. Kramer, F. R. N. Schneider, S. T. Ohlmann +4

Common envelope (CE) phases in binary systems where the primary star reaches the tip of the red giant branch are discussed as a formation scenario for hot subluminous B-type (sdB)…

astro-ph.SR2020★ 21 cited

An in-depth reanalysis of the alleged type Ia supernova progenitor Henize 2-428

N. Reindl, V. Schaffenroth, M. M. Miller Bertolami +5

The nucleus of the planetary nebula Hen2-428 is a short orbital-period (4.2h), double-lined spectroscopic binary, whose status as a potential supernova type Ia progenitor has raise…