activity
19972007
most citedWhite Dwarf Mass Distribution in the SDSS

329 citations · 675 across the 6 of their papers we have counts for

collaborators

6 papers

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-ph2007★ 329 cited

White Dwarf Mass Distribution in the SDSS

S. O. Kepler, S. J. Kleinman, A. Nitta +5

We determined masses for the 7167 DA and 507 DB white dwarf stars classified as single and non-magnetic in data release four of the Sloan Digital Sky Survey (SDSS). We obtained rev…

astro-ph2006★ 46 cited

Towards a pure ZZ Ceti instability strip

B. G. Castanheira, S. O. Kepler, A. F. M. Costa +8

We have observed again two stars inside the ZZ Ceti instability strip that were previously classified as not-observed-to-vary (NOV) by Mukadam et al. (2004) and found them to be lo…

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-ph2001★ 49 cited

Discover of the "missing" mode in HR 1217 by the Whole Earth Telescope

D. W. Kurtz, S. D. Kawaler, R. L. Riddle et al.

HR 1217 is a prototypical rapidly oscillating Ap star that has presented a test to the theory of nonradial stellar pulsation. Prior observations showed a clear pattern of five mode…

astro-ph1997★ 119 cited

Understanding the Cool DA White Dwarf, G29-38

S. J. Kleinman, R. E. Nather, D. E. Winget +37

The white dwarfs are promising laboratories for the study of cosmochronology and stellar evolution. Through observations of the pulsating white dwarfs, we can measure their interna…