activity
20052009
most citedSpectral analyses of eighteen hot H-deficient (pre-) white dwarfs from the Sloan Digital Sky Survey Data Release 4

45 citations · 108 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2009★ 4 cited

Non-LTE spectral analyses of the lately discovered DB-gap white dwarfs from the SDSS

S. D. Huegelmeyer, S. Dreizler

For a long time, no hydrogen-deficient white dwarfs have been known that have effective temperature between 30 kK and < 45 kK, i.e. exceeding those of DB white dwarfs and having lo…

astro-ph.SR2009

Spectral synthesis of circumstellar disks - application to white dwarf debris disks

S. D. Huegelmeyer, S. Dreizler, D. Homeier +1

Gas and dust disks are common objects in the universe and can be found around various objects, e.g. young stars, cataclysmic variables, active galactic nuclei, or white dwarfs. The…

astro-ph.SR2009★ 25 cited

The planet-hosting subdwarf B star V391 Pegasi is a hybrid pulsator

R. Lutz, S. Schuh, R. Silvotti +4

A noticeable fraction of subdwarf B stars shows either short-period (p-mode) or long-period (g-mode) luminosity variations, with two objects so far known to exhibit hybrid behaviou…

astro-ph2007

Light curve analysis of the hybrid sdB pulsators HS0702+6043 and HS2201+2610

R. Lutz, S. Schuh, R. Silvotti +6

We present the detection of low-amplitude, long-period g-modes in two individual sdBV stars which are known to be p-mode pulsators. Only few of these hybrid objects, showing both p…

astro-ph2007★ 21 cited

Investigation of transit-selected exoplanet candidates from the MACHO survey

S. D. Huegelmeyer, S. Dreizler, D. Homeier +1

Context: Planets outside our solar system transiting their host star, i. e. those with an orbital inclination near 90 degree, are of special interest to derive physical properties…

astro-ph2006

Observational constraints on the evolutionary connection between PG 1159 stars and DO white dwarfs

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

The Sloan Digital Sky Survey has provided spectra of a large number of new PG 1159 stars and DO white dwarfs. This increase in known hot H-deficient compact objects significantly i…