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The Period Change Rate in the RS CVn Binary HD 5303

  • K. Thompson (a1), D. W. Coates (a1) and G. Anders (a1)

Abstract

From the observed timings of primary eclipse of HD 5303 we find that its 2.7 day period is increasing at a rate of about one second per year. In this paper we consider the implications of this in terms of mass transfer or mass loss from the system.

Copyright

COPYRIGHT: © Astronomical Society of Australia 1991

References

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The Period Change Rate in the RS CVn Binary HD 5303

  • K. Thompson (a1), D. W. Coates (a1) and G. Anders (a1)

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