activity
19962013
most citedOrbital periods of twenty two subdwarf B stars

156 citations · 1.5k across the 44 of their papers we have counts for

collaborators

45 papers

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.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…

astro-ph.SR2011

Helium abundances and the helium isotope anomaly of sdB stars

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

Helium abundances and atmospheric parameters have been determined from high resolution spectra for a new sample of 46 bright hot subdwarf B (sdB) stars. The helium abundances have…

astro-ph.SR2011★ 54 cited

PG1018-047: the longest period subdwarf B binary

J. Deca, T. R. Marsh, R. H. Østensen +7

About 50% of all known hot subdwarf B stars (sdBs) reside in close (short period) binaries, for which common envelope ejection is the most likely formation mechanism. However, Han…

astro-ph.SR2011★ 108 cited

Radial velocity measurements of Subdwarf B stars

C. M. Copperwheat, L. Morales-Rueda, T. R. Marsh +2

Subdwarf B (sdB) stars are hot, sub-luminous stars which are thought to be core-helium burning with thin hydrogen envelopes. The mechanism by which these stars lose their envelopes…

astro-ph.SR2009★ 47 cited

Discovery of a close substellar companion to the hot subdwarf star HD 149382 - The decisive influence of substellar objects on late stellar evolution

S. Geier, H. Edelmann, U. Heber +1

Substellar objects, like planets and brown dwarfs orbiting stars, are by-products of the star formation process. The evolution of their host stars may have an enourmous impact on t…