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19992007
most citedEvolutionary calculations of phase separation in crystallizing white dwarf stars

73 citations · 281 across the 6 of their papers we have counts for

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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★ 12 cited

Near-Infrared Molecular Hydrogen Emission from the Central Regions of Galaxies: Regulated Physical Conditions in the Interstellar Medium

Soojong Pak, D. T. Jaffe, G. J. Stacey +3

The central regions of many interacting and early-type spiral galaxies are actively forming stars. This process affects the physical and chemical properties of the local interstell…

astro-ph2003★ 50 cited

Observations of the pulsating subdwarf B star Feige 48: Constraints on evolution and companions

M. D. Reed, S. D. Kawaler

Since pulsating subdwarf B (sdBV or EC14026) stars were first discovered (Kilkenny et al, 1997), observational efforts have tried to realize their potential for constraining the in…

astro-ph2003★ 66 cited

The Everchanging Pulsating White Dwarf GD358

S. O. Kepler, R. E. Nather, D. E. Winget +43

We report 323 hours of nearly uninterrupted time series photometric observations of the DBV star GD 358 acquired with the Whole Earth Telescope (WET) during May 23rd to June 8th, 2…

astro-ph1999★ 73 cited

Evolutionary calculations of phase separation in crystallizing white dwarf stars

M. H. Montgomery, E. W. Klumpe, D. E. Winget +1

We present an exploration of the significance of Carbon/Oxygen phase separation in white dwarf stars in the context of self-consistent evolutionary calculations. Because phase sepa…