No CrossRef data available.
Article contents
Analysis of Long-Term Single-Site Observations of The Pulsating DB White Dwarf GD 3581
Published online by Cambridge University Press: 12 April 2016
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
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
- Information
- International Astronomical Union Colloquium , Volume 193: Variable Stars in the Local Group , 2004 , pp. 506 - 510
- Copyright
- Copyright © Astronomical Society of the Pacific 2004
Footnotes
1
These data were collected at McDonald Observatory, Fort Davis, Texas
References
Nather, R.E., Winget, D.E., Clemens, J.C, Hansen, C.J., Hine, B.P.
1990
ApJ, 361, 309
CrossRefGoogle Scholar
You have
Access