activity
19972008
most citedUnderstanding the Cool DA White Dwarf, G29-38

119 citations · 755 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph2008★ 33 cited

New Pulsating DB White Dwarf Stars from the Sloan Digital Sky Survey

A. Nitta, S. J. Kleinman, J. Krzesinski +8

We are searching for new He atmosphere white dwarf pulsators (DBVs) based on the newly found white dwarf stars from the spectra obtained by the Sloan Digital Sky Survey. DBVs pulsa…

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-ph2005★ 87 cited

Measuring the evolution of the most stable optical clock G 117-B15A

S. O. Kepler, J. E. S. Costa, B. G. Castanheira +7

We report our measurement of the rate of change of period with time dP/dt for the 215 s periodicity in the pulsating white dwarf G 117-B15A, the most stable optical clock known. Af…

astro-ph2005★ 12 cited

An asteroseismic test of diffusion theory in white dwarfs

T. S. Metcalfe, R. E. Nather, T. K. Watson +3

The helium-atmosphere (DB) white dwarfs are commonly thought to be the descendants of the hotter PG1159 stars, which initially have uniform He/C/O atmospheres. In this evolutionary…

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…