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20022024
most citedOn the Purity of the ZZ Ceti Instability Strip: Discovery of More Pulsating DA White Dwarfs on the Basis of Optical Spectroscopy

127 citations · 623 across the 21 of their papers we have counts for

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6 papers · 1 filter

astro-ph2007★ 11 cited

Discovery of a bright eclipsing cataclysmic variable

D. K. Sing, E. M. Green, S. B. Howell +4

We report on the discovery of J0644+3344, a bright deeply eclipsing cataclysmic variable (CV) binary. Spectral signatures of both binary components and an accretion disk can be see…

astro-ph2005★ 1 cited

Exciting new features in the frequency spectrum of the EC14026 star HS0702+6043 - Simultaneous g-modes and p-modes in a sdB pulsator

S. Schuh, J. Huber, S. Dreizler +7

The discovery of a long-period g-mode oscillation in the previously known short-period p-mode sdB pulsator HS0702+6043 makes this star an extraordinary object, unique as a member o…

astro-ph2005★ 103 cited

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★ 83 cited

Structural Parameters of the Hot Pulsating B Subdwarf PG 1219+534 from Asteroseismology

S. Charpinet, G. Fontaine, P. Brassard +2

We have carried out a detailed asteroseismic analysis of PG 1219+534. Our analysis leads to the identification of the (k,l) indices of nine periods observed in the star PG 1219+534…

astro-ph2003★ 127 cited

On the Purity of the ZZ Ceti Instability Strip: Discovery of More Pulsating DA White Dwarfs on the Basis of Optical Spectroscopy

P. Bergeron, G. Fontaine, M. Billeres +2

We report the discovery of two new ZZ Ceti pulsators, LP 133-144 and HE 1258+0123, selected on the basis of model atmosphere fits to optical spectroscopic data. The atmospheric par…

astro-ph2002★ 72 cited

Resolving subdwarf B stars in binaries by HST imaging

U. Heber, S. Moehler, R. Napiwotzki +2

The origin of subluminous B stars is still an unsolved problem in stellar evolution. Single star as well as close binary evolution scenarios have been invoked but until now have me…