Hostname: page-component-cd9895bd7-gvvz8 Total loading time: 0 Render date: 2024-12-26T04:04:01.359Z Has data issue: false hasContentIssue false
  • English
  • Français

Minimum-Light Phenomena in Nova-like Variables

Published online by Cambridge University Press:  12 April 2016

George S. Mumford
George S. Mumford*
Affiliation:
Medford, Tucson

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.

Some characteristics of the small-amplitude, quasi-periodic light fluctuations common to novalike variables are described. There appears to be a weak correlation for the majority of the objects between the dispersion about the mean magnitude and the interval between outbursts such that systems with infrequent outbursts exhibit the largest dispersions.

Type
IV. Duplicity and its Consequences among the Intrinsic Variable Stars
Information
International Astronomical Union Colloquium , Volume 15: New Directions and Frontiers in Variable Stars Research , 1971 , pp. 275 - 278
Copyright
Copyright © Cambridge University Press 1971

References

Mumford, G. S., 1966, Ap. J. 146, 411.CrossRefGoogle Scholar
Mumford, G. S., 1967, P.A.S.P. 79, 283.CrossRefGoogle Scholar
Mumford, G. S., 1971, Ap. J. 165, 369.CrossRefGoogle Scholar
Walker, M. F., 1961, Ap. J., 134, 171.CrossRefGoogle Scholar