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20012020
most citedOrbital periods of twenty two subdwarf B stars

156 citations · 1.4k across the 50 of their papers we have counts for

collaborators

49 papers

astro-ph.SR2020★ 26 cited

Hypervelocity Stars in the Gaia era. Revisiting the most extreme stars from the MMT survey

S. Kreuzer, A. Irrgang, U. Heber

The hypervelocity star (HVS) survey conducted at the Multiple Mirror Telescope (MMT) identified 42 B-type stars in the Galactic halo whose radial velocity in the Galactic rest-fram…

astro-ph.SR2016

Close binary progenitors and ejected companions of thermonuclear supernovae

S. Geier, T. Kupfer, U. Heber +8

Hot subdwarf stars (sdO/Bs) are evolved core helium-burning stars with very thin hydrogen envelopes, which can be formed by common envelope ejection. Close sdB binaries with massiv…

astro-ph.SR2016

Hot subdwarf stars and their connection to thermonuclear supernovae

S. Geier, T. Kupfer, E. Ziegerer +4

Hot subdwarf stars (sdO/Bs) are evolved core helium-burning stars with very thin hydrogen envelopes, which can be formed by common envelope ejection. Close sdB binaries with massiv…

astro-ph.SR2015★ 121 cited

Hot subdwarf binaries from the MUCHFUSS project - Analysis of 12 new systems and a study of the short-period binary population

T. Kupfer, S. Geier, U. Heber +6

The project Massive Unseen Companions to Hot Faint Underluminous Stars from SDSS (MUCHFUSS) aims at finding hot subdwarf stars with massive compact companions like massive white dw…

astro-ph.SR2014★ 1 cited

New HW Virginis Systems from the MUCHFUSS Project

V. Schaffenroth, S. Geier, I. Barbu-Barna +3

In course of the MUCHFUSS project we found two new HW Virginis systems. J192059+372220 (J1920) has an orbital period of 0.169 d and an M dwarf companion with a mass of $0.116 M_{\o…

astro-ph.SR2014★ 1 cited

The mysterious sdO X-ray binary BD+37 442

U. Heber, S. Geier, A. Irrgang +4

Pulsed X-ray emission in the luminous, helium-rich sdO BD+37 442 has recently been discovered (La Palombara et al., 2012). It was suggested that the sdO star has a neutron star or…