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Analysis of Long-Term Single-Site Observations of The Pulsating DB White Dwarf GD 3581

Published online by Cambridge University Press:  12 April 2016

P.A. Bradley*
Affiliation:
Los Alamos National Laboratory, X-2 MS B220, Los Alamos, NM 87545-2345, USA

Abstract

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We briefly describe the analysis of single-site data collected from 1982 to 1992 for the pulsating DB white dwarf GD 358. We show that the amplitudes of almost all of the l = 1 modes change over time, and some of the l = 1 modes disappear for months at a time. We also find a new mode at k = 19, with a frequency of ~1173μHz.

Type
Part 9. Evolutionary and pulsation properties of variable stars
Copyright
Copyright © Astronomical Society of the Pacific 2004

Footnotes

1

These data were collected at McDonald Observatory, Fort Davis, Texas

References

Bradley, P.A., Winget, D.E. 1994 ApJ, 430, 850 CrossRefGoogle Scholar
Brickhill, J.A. 1992 MNRAS, 259, 529 CrossRefGoogle Scholar
Clemens, J.C. 1993 Baltic Astron., 2, 511 Google Scholar
Kepler, S.O. 1993 Baltic Astron., 2, 515 Google Scholar
Kepler, S.O. et al. 2003 A&A, 401, 639 Google Scholar
Nather, R.E., Winget, D.E., Clemens, J.C, Hansen, C.J., Hine, B.P. 1990 ApJ, 361, 309 CrossRefGoogle Scholar
Vuille, F., et al. 2000 MNRAS, 314, 689 Google Scholar
Winget, D.E., et al. 1994 ApJ, 430, 839 Google Scholar
Wu, Y. 2001 MNRAS, 323, 248 Google Scholar