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An Analysis of the Light Curves of Z Cha

Published online by Cambridge University Press:  12 April 2016

J. Smak
J. Smak*
Affiliation:
Copernicus Astronomical Center, Polish Academy of Sciences, Warsaw, Poland

Extract

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Photometric results by Warner (.1974) and Bailey (1979) are re-analysed to derive geometrical and relative photometric parameters of the system at minimum light. Relative mass of the secondary component is found between μ = 0.1 and 0.2, while its photometric contribution at the bottom of eclipse is between 20 and 40 percent.

Type
Abstracts of Workshop Papers on Dwarf Novae
Information
International Astronomical Union Colloquium , Volume 53: White Dwarfs and Variable Degenerate Stars , August 1979 , pp. 502
Copyright
Copyright © The University of Rochester 1979

References

Bailey, J. 1979, M.N.R.A.S., in press.Google Scholar
Warner, B. 1974, M.N.R.A.S., 168, 235.CrossRefGoogle Scholar