activity
19962022
most citedHubble Space Telescope Spectroscopy of V471 Tauri: Oversized K Star, Paradoxical White Dwarf

122 citations · 670 across the 14 of their papers we have counts for

collaborators

13 papers

astro-ph.HE2022★ 37 cited

Localised thermonuclear bursts from accreting magnetic white dwarfs

S. Scaringi, P. J. Groot, C. Knigge +16

Nova explosions are caused by global thermonuclear runaways triggered in the surface layers of accreting white dwarfs. It has been predicted that localised thermonuclear bursts on…

astro-ph2008★ 29 cited

Whole Earth Telescope observations of the hot helium atmosphere pulsating white dwarf EC 20058-5234

WET Collaboration, D. J. Sullivan, T. S. Metcalfe +22

We present the analysis of a total of 177h of high-quality optical time-series photometry of the helium atmosphere pulsating white dwarf (DBV) EC 20058-5234. The bulk of the observ…

astro-ph2007★ 53 cited

The pulsation modes of the pre-white dwarf PG 1159-035

J. E. S. Costa, S. O. Kepler, D. E. Winget +74

PG 1159-035, a pre-white dwarf with T_eff=140,000 K, is the prototype of both two classes: the PG1159 spectroscopic class and the DOV pulsating class. Previous studies of PG 1159-0…

astro-ph2006★ 27 cited

Whole Earth Telescope observations of the pulsating subdwarf B star PG 0014+067

M. Vuckovic, S. D. Kawaler

PG 0014+067 is one of the most promising pulsating subdwarf B stars for seismic analysis, as it has a rich pulsation spectrum. The richness of its pulsations, however, poses a fund…

astro-ph2004★ 79 cited

Whole Earth Telescope observations of BPM 37093: a seismological test of crystallization theory in white dwarfs

A. Kanaan, A. Nitta, D. E. Winget +3

BPM 37093 is the only hydrogen-atmosphere white dwarf currently known which has sufficient mass (~ 1.1 M_sun) to theoretically crystallize while still inside the ZZ Ceti instabilit…

astro-ph2002★ 76 cited

FIRST J102347.6+003841: The First Radio-Selected Cataclysmic Variable

Howard E. Bond, Richard L. White, Robert H. Becker +1

We have identified the 1.4 GHz radio source FIRST J102347.6+003841 (hereafter FIRST J1023+0038) with a previously unknown 17th-mag Galactic cataclysmic variable (CV). The optical s…