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Klaus Werner

Researcher at University of Tübingen

Publications -  449
Citations -  7926

Klaus Werner is an academic researcher from University of Tübingen. The author has contributed to research in topics: White dwarf & Stars. The author has an hindex of 44, co-authored 433 publications receiving 7353 citations. Previous affiliations of Klaus Werner include Max Planck Society & University of Potsdam.

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The Element Abundances in Bare Planetary Nebula Central Stars and the Shell Burning in AGB Stars

Klaus Werner, +1 more
- 13 Dec 2005 - 
TL;DR: In this article, the observed properties of extremely hot hydrogen-deficient post-AGB stars of spectral type [WC] and PG1159 were reviewed, and the state-of-the-art stellar evolution models which simulate AGB evolution and the occurrence of a late He-shell flash were summarized.
Journal ArticleDOI

The Elemental Abundances in Bare Planetary Nebula Central Stars and the Shell Burning in AGB Stars

TL;DR: In this article, the observed properties of extremely hot, hydrogen-deficient post-asymptotic giant branch (AGB) stars of spectral type (WC) and PG1159 were reviewed.
Journal ArticleDOI

Is RX J1856.5-3754 a Quark Star?

TL;DR: In this paper, Chandra Low Energy Transmission Grating and High Resolution Camera spectroscopic observations of the isolated neutron star candidate RX J1856.5-3754 have been analyzed to search for metallic and resonance cyclotron spectral features and for pulsation behavior.
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A neutron star stiff equation of state derived from cooling phases of the x-ray burster 4u 1724–307

TL;DR: In this article, an improved method of determining the basic stellar parameters using the data from the cooling phase of photospheric radius expansion (PRE) bursts covering a large range of luminosities was proposed.
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Is RX J185635-375 a Quark Star?

TL;DR: In this article, the authors used deep Chandra-HRC-S observations of the isolated neutron star candidate RX J1856.5-3754 to search for metallic and resonance cyclotron spectral features and for pulsation behaviour.