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An Analysis of the Light Curves of Z Cha
Published online by Cambridge University Press: 12 April 2016
Extract
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