most citedHST and FUSE Spectroscopy of Hot Hydrogen-Rich Central Stars of Planetary Nebulae

2 citations · 4 across the 12 of their papers we have counts for

collaborators

11 papers

cs.CR2005

Security for Distributed Web-Applications via Aspect-Oriented Programming

Nicolai Kuntze, Thomas Rauch, Andreas U. Schmidt

Identity Management is becoming more and more important in business systems as they are opened for third parties including trading partners, consumers and suppliers. This paper pre…

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…

astro-ph2004

Iron Abundance in Hydrogen-Rich Central Stars of Planetary Nebulae

A. I. D. Hoffmann, I. Traulsen, T. Rauch +3

We report on an on-going analysis of high-resolution UV spectra of hot hydrogen-rich central stars of planetary nebulae (CSPN), obtained with the Hubble Space Telescope and FUSE. S…

astro-ph20042 cited

HST and FUSE Spectroscopy of Hot Hydrogen-Rich Central Stars of Planetary Nebulae

I. Traulsen, A. I. D. Hoffmann, T. Rauch +3

High-resolution UV spectra, obtained with HST and FUSE, enable us to analyse hot hydrogen-rich central stars in detail. Up to now, optical hydrogen and helium lines have been used…

astro-ph2004

FUSE spectroscopy of PG1159 Stars

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

PG1159 stars are hot hydrogen-deficient post-AGB stars with effective temperatures within a range from 75000 K up to 200000 K. These stars are probably the result of a late helium-…

astro-ph2004

Spectral Analysis of Super Soft X-ray Sources: V4743 Sagittarii

Thomas Rauch, Marina Orio, R. Gonzales-Riestra +1

Half a year after its outburst, the nova V4743 Sgr evolved into the brightest super-soft X-ray source in the sky with a flux maximum around 30A, exhibiting resonance lines of C V,…