activity
19982007
most citedHS2237+8154: On the onset of mass transfer or entering the period gap?

54 citations · 147 across the 18 of their papers we have counts for

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Showing 2002Show all

9 papers · 1 filter

astro-ph2002

Towards asteroseismology of the non-radial pulsating sdB star PG 1605+072

S. Falter, U. Heber, S. Dreizler +2

The recently discovered new class of sdB pulsators (sdBV) offers a powerful possibility for the investigation of their interior and thus their evolutionary history. The first step…

astro-ph20021 cited

Photometric and Spectroscopic Monitoring of the sdBV star PG 1605+072: The Multi-Site Spectroscopic Telescope (MSST) Project

U. Heber, S. Dreizler, S. L. Schuh +2

A small fraction of subluminous B stars show short-period, multiperiodic light variations and form the new class of pulsating star known as EC 14026 variables, after the prototype.…

astro-ph20021 cited

The Rotational Velocity of Helium-rich Pre-White Dwarfs

T. Rauch, S. Koeper, S. Dreizler +3

Previous investigations on hydrogen-rich white dwarfs generally yield only very small rotational velocities (v_rot sin i). We have analyzed line profiles in high-resolution optical…

astro-ph200222 cited

Model Photospheres with Accelerated Lambda Iteration

K. Werner, J. L. Deetjen, S. Dreizler +3

We address the classical stellar-atmosphere problem and describe our method of numerical solution in detail. The problem consists of the solution of the radiation transfer equation…

astro-ph2002

FUSE Spectroscopy of the Two Prototype White Dwarfs With Signatures of a Super-hot Wind

K. Werner, S. Dreizler, J. W. Kruk +1

The O VIII phenomenon describes the occurrence of ultra-high ionization absorption lines of the CNO elements (e.g. O VIII, N VII, C VI, and even Ne X) in the optical spectra hot of…

astro-ph2002

Metal abundances in PG1159 stars from Chandra and FUSE spectroscopy

K. Werner, J. L. Deetjen, S. Dreizler +3

We investigate FUSE spectra of three PG1159 stars and do not find any evidence for iron lines. From a comparison with NLTE models we conclude a deficiency of 1-1.5 dex. We speculat…