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 2005Show all

7 papers · 1 filter

astro-ph2005

HS0702+6043: A star showing both short-period p-mode and long-period g-mode oscillations

S. Schuh, J. Huber, S. Dreizler +4

[Context.] The hot subdwarf B star HS0702+6043 is known as a large-amplitude, short-period p-mode pulsator of the EC14026 type. Its atmospheric parameters place it at the common bo…

astro-ph2005

On the most metal-poor PN and its binary central star

R. Napiwotzki, G. Tovmassian, M. G. Richer +5

PN G135.9+55.9 is the most metal-poor PN known in our Galaxy. The central star resides in a short-period binary system with a compact component, probably a white dwarf. We describe…

astro-ph200513 cited

Spectral analyses of DO white dwarfs and PG1159 stars from the Sloan Digital Sky Survey

S. D. Huegelmeyer, S. Dreizler, K. Werner +3

We present a model atmosphere analysis of ten new DO white dwarfs and five new PG 1159 stars discovered in the Sloan Digital Sky Survey DR1, DR2 and DR3. This is a significant incr…

astro-ph2005

Light and heavy metal abundances in hot central stars of planetary nebulae

K. Werner, A. I. D. Hoffmann, D. Jahn +5

We present new results from our spectral analyses of very hot central stars achieved since the last IAU Symposium on planetary nebulae held in Canberra 2001. The analyses are mainl…

astro-ph2005

The MultiSite Spectroscopic Telescope campaign: 2m spectroscopy of the V361 Hya variable PG1605+072

S. J. O'Toole, U. Heber, C. S. Jeffery +10

We present results and analysis for the 2m spectroscopic part of the MultiSite Spectroscopic Telescope (MSST) campaign undertaken in May/June 2002. The goal of the project was to o…

astro-ph20051 cited

The Spectral Variability of Pulsating Stars: PG1159-035

T. Stahn, S. Dreizler, K. Werner

With 10m class telescopes as well as with time-tagging detectors on board of HST and FUSE, the analysis of time-resolved spectra for pulsating white dwarfs becomes feasible. We pre…