activity
20012024
most citedHE 0437-5439 -- an unbound hyper-velocity main-sequence B-type star

191 citations · 828 across the 26 of their papers we have counts for

collaborators

26 papers

astro-ph.IM2024★ 11 cited

Archives of Photographic PLates for Astronomical USE (APPLAUSE) Digitisation of astronomical plates and their integration into the International Virtual Observatory

Harry Enke, Taavi Tuvikene, Detlef Groote +2

The Archives of Photographic PLates for Astronomical USE (APPLAUSE) project is aimed at digitising astronomical photographic plates from three major German plate collections, makin…

astro-ph.SR2014★ 23 cited

Two candidate brown dwarf companions around core helium-burning stars

V. Schaffenroth, L. Classen, K. Nagel +4

Hot subdwarf stars of spectral type B (sdBs) are evolved, core helium-burning objects. The formation of those objects is puzzling, because the progenitor star has to lose almost it…

astro-ph.SR2014★ 26 cited

Orbital solutions of eight close sdB binaries and constraints on the nature of the unseen companions

S. Geier, R. H. Oestensen, U. Heber +9

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

astro-ph.SR2013★ 16 cited

Hot subdwarf stars in close-up view IV. Helium abundances and the He isotopic anomaly of subdwarf B star

S. Geier, U. Heber, H. Edelmann +5

Atmospheric parameters and helium abundances of 44 bright subdwarf B stars have been determined. More than half of our sample consists of newly discovered stars from the Edinburgh…

astro-ph.SR2013★ 26 cited

The subdwarf B star SB 290 - A fast rotator on the extreme horizontal branch

S. Geier, U. Heber, C. Heuser +3

Hot subdwarf B stars (sdBs) are evolved core helium-burning stars with very thin hydrogen envelopes. In order to form an sdB, the progenitor has to lose almost all of its hydrogen…

astro-ph.SR2011★ 1 cited

Low-mass stellar and substellar companions to sdB stars

S. Geier, L. Classen, P. Bruenner +9

It has been suggested that besides stellar companions, substellar objects in close orbits may be able to trigger mass loss in a common envelope phase and form hot subdwarfs. In an…