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20002008
most citedMonster Redshift Surveys through Dispersive Slitless Imaging: The Baryon Oscillation Probe

17 citations · 19 across the 15 of their papers we have counts for

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astro-ph2008

UV and FUV spectroscopy of the hybrid PG 1159-type central star NGC 7094

M. Ziegler, T. Rauch, E. Reiff +3

Previous studies aiming at the iron-abundance determination in three PG 1159 stars (K 1-16, PG 1159-035, NGC 7094) and a [WC]-PG 1159 transition star (Abell 78) have revealed that…

astro-ph2008

Search For Iron, Nickel, and Fluorine in PG1159 Stars

E. Reiff, T. Rauch, K. Werner +2

A possible origin of the iron-deficiency in PG1159 stars could be neutron captures on Fe nuclei. A nickel overabundance would corroborate this idea. Consequently we are looking for…

astro-ph2007

KPD0005+5106: Hottest DO White Dwarf Much Hotter Than Assumed

K. Werner, T. Rauch, J. W. Kruk

KPD0005+5106 is the hottest known helium-rich white dwarf. We have identified NeVIII lines in UV and optical spectra and conclude that it is significantly hotter than previously th…

astro-ph2007

Elemental Abundances in PG1159 Stars

K. Werner, T. Rauch, E. Reiff +1

The hydrogen-deficiency in extremely hot post-AGB stars of spectral class PG1159 is probably caused by a (very) late helium-shell flash or a AGB final thermal pulse that consumes t…

astro-ph2007

Spectral Analysis of Central Stars of Planetary Nebulae

Thomas Rauch, Klaus Werner, Marc Ziegler +2

Spectral analysis by means of NLTE model atmospheres has presently arrived at a high level of sophistication. High-resolution spectra of central stars of planetary nebulae can be r…

astro-ph2004

Fluorine in extremely hot post-AGB stars

K. Werner, T. Rauch, J. W. Kruk

We have discovered lines of highly ionized fluorine (Fv and Fvi) in the far-UV spectra of extremely hot (Teff=85,000--150,000 K) post-AGB stars. Our sample comprises H-rich central…