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8. High Frequency Stellar Oscillations: IV: Photoelectric Monitoring of Southern White Dwarfs

Published online by Cambridge University Press:  14 August 2015

J. E. Hesser  and
B. M. Lasker
J. E. Hesser
Affiliation:
Cerro Tololo Inter-American Observatory∗, La Serena, Chile
B. M. Lasker
Affiliation:
Cerro Tololo Inter-American Observatory∗ and The University of Michigan

Abstract

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Time-series data for 14 stars in the list of Eggen and Greenstein have been used to compute their power spectra, which confirm previously found quiescency in the 4 to 700 sec period range. Additionally, characteristics of the continuous power spectra are considered.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 42: White Dwarfs , 1971 , pp. 41 - 45
Copyright
Copyright © Reidel 1971 

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