papers

Publications (23)

astro-ph.SR2013

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-ph2003

Simultaneous time-series spectroscopy and multi-band photometry of the sdBV PG 1605+072

S. Falter, U. Heber, S. Dreizler +3

We present time-series spectroscopy and multi-band photometry of the sdBV PG 1605+072 carried out simultaneously at the Calar Alto 2.2m and 3.5m telescopes. The periodogram analysi…

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-ph2001

Binaries discovered by the SPY project I. HE 1047-0436: a subdwarf B + white dwarf system

R. Napiwotzki, H. Edelmann, U. Heber +4

In the course of our search for double degenerate binaries as potential progenitors of type Ia supernovae with the UVES spectrograph at the ESO VLT (ESO SN Ia Progenitor surveY - S…

astro-ph2003

Spectral analysis of sdB stars from the Hamburg Quasar Survey

H. Edelmann, U. Heber, H. -J. Hagen +4

We present the results of a spectral analysis of a large sample of subdwarf B stars selected from follow-up observations of candidates from the Hamburg Quasar Survey. Fundamental p…

astro-ph.SR2014

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-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-ph.SR2011

Rotational properties of single and wide binary subdwarf B stars

S. Geier, U. Heber, H. Edelmann +2

We measured projected rotational velocities of more than a hundred apparently single sdBs. A comparison is made with sdB stars in binary systems with orbits so wide, that tidal int…

astro-ph2001

Early type stars at high galactic latitudes II. Four evolved B-type stars of unusual chemical composition

M. Ramspeck, U. Heber, H. Edelmann

We present the result of differential spectral analyses of a further four apparently normal B-type stars. Abundance anomalies (e.g. He, C, N enrichment), slow rotation and/or high…

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…

astro-ph.SR2014

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-ph2008

KBS 13 -- a Rare Reflection Effect sdB Binary with an M Dwarf Secondary

B. -Q. For, H. Edelmann, E. M. Green +3

We report preliminary VRI differential photometric and spectroscopic results for KBS 13, a recently discovered non-eclipsing sdB+dM system. Radial velocity measurements indicate an…

astro-ph2002

Discovery of A New Class of Pulsating Stars: Gravity-mode Pulsators among Subdwarf B Stars

E. M. Green, G. Fontaine, M. D. Reed +15

During the course of an ongoing CCD monitoring program to investigate low-level light variations in subdwarf B (sdB) stars, we have serendipitously discovered a new class of low am…

astro-ph2005

NLTE analyses of sdB stars: progress and prospects

N. Przybilla, M. F. Nieva, H. Edelmann

We report on preliminary results of a hybrid non-LTE analysis of high-resolution, high-S/N spectra of the helium-rich subdwarf B star Feige49 and the helium-poor sdB HD205805. Non-…

astro-ph.SR2013

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-ph2007

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 - Four Candidate Systems with Neutron Star/Black Hole Companions Discovered

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-ph.SR2009

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…

astro-ph.SR2010

Hot subdwarf stars in close-up view I. Rotational properties of subdwarf B stars in close binary systems and nature of their unseen companions

S. Geier, U. Heber, Ph. Podsiadlowski +4

The origin of hot subdwarf B stars (sdBs) is still unclear. About half of the known sdBs are in close binary systems for which common envelope ejection is the most likely formation…

astro-ph.SR2011

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-ph2008

LMC origin of the hyper-velocity star HE 0437-5439. Beyond the supermassive black hole paradigm

N. Przybilla, M. F. Nieva, U. Heber +4

Context: Hyper-velocity stars move so fast that only a supermassive black hole (SMBH) seems to be capable to accelerate them. Hence the Galactic centre (GC) is their only suggested…

astro-ph2003

Studying the populations of our Galaxy using the kinematics of sdB stars

M. Altmann, H. Edelmann, K. S. de Boer

We have analysed the kinematics of a sample of 114 hot subdwarf stars, for 2/3 of which we present new proper motions, spectroscopic and photometric data. The vast majority of the…

astro-ph2005

High resolution spectroscopy of bright subdwarf B stars - I. Radial velocity variables

H. Edelmann, U. Heber, M. Altmann +2

Radial velocity curves for 15 bright subdwarf B binary systems have been measured using high precision radial velocity measurements from high S/N optical high-resolution spectra. I…