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Rapid Balmer Line Variability in Ap Stars

Published online by Cambridge University Press:  12 April 2016

H. John Wood
H. John Wood*
Affiliation:
ESO-Chile

Extract

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It is the purpose of this paper to briefly summarize the results of an eight-year observational program on the Balmer-line behavior of magnetic and related stars. In addition, new data on the interesting 79-minute variable SX Phe will be presented.

Type
III. Rapid and Ultrarapid Variables (Including X-Rax Sources)
Information
International Astronomical Union Colloquium , Volume 15: New Directions and Frontiers in Variable Stars Research , 1971 , pp. 176 - 177
Copyright
Copyright © Cambridge University Press 1971