activity
20062008
most citedHypervelocity Stars: Young and Heavy or Old and Light?

2 citations · 4 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph20081 cited

HW Vir's Companion: a M-type Dwarf, or maybe a giant rotating spherical Mirror?

Heinz Edelmann

From optical high-resolution spectra the nature of the unseen companion of HW Vir is determined without detection of any spectral features originating from the secondary itself. Us…

astro-ph20082 cited

Hypervelocity Stars: Young and Heavy or Old and Light?

Uli Heber, Heiko Hirsch, Heinz Edelmann +4

The first three hyper-velocity stars (HVS) unbound to the Galaxy were serendipitously discovered in 2005. The only suggested origin of hyper-velocity stars is the Galactic Centre a…

astro-ph2008

Binary sdB Stars with Massive Compact Companions

S. Geier, C. Karl, H. Edelmann +2

The masses of compact objects like white dwarfs, neutron stars and black holes are fundamental to astrophysics, but very difficult to measure. We present the results of an analysis…

astro-ph20071 cited

Tidal synchronization of the subdwarf B binary PG 0101+039

S. Geier, S. Nesslinger, U. Heber +3

Tidally locked rotation is a frequently applied assumption that helps to measure masses of invisible compact companions in close binaries. The calculations of synchronization times…

astro-ph2006

Spectroscopic Analysis of subluminous B Stars in Binaries with compact Companions

S. Geier, C. Karl, H. Edelmann +2

The masses of compact objects like white dwarfs, neutron stars and black holes are fundamental to astrophysics, but very difficult to measure. We present the results of an analysis…