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Z Andromedae

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Z Andromedae is the class prototype of the symbiotic stars, binary stars consisting of a red giant donor star and a hot accreting star, either a white dwarf or neutron star.  The most prominent features of the Z Andromedae light curve shown here are the outbursts that occur roughly every 600 days.  In the case of Z Andromedae, the optical light of these outbursts arises from two processes: an outburst of an accretion disk around the white dwarf, and from thermonuclear burning on the surface of the white dwarf itself.  The latter is a similar process as what happens in the classical novae, but at a much slower rate.

The outbursts of Z Andromedae do not occur with the same frequency as the orbital period -- recent outbursts have occurred between 600 and 700 days apart, but the orbital period is slightly longer, about 750 days.  Leibowitz and Formiggini (2008) suggest that the outburst period is a beat period between this orbital period and a longer cycle, perhaps similar to the 11-year solar-activity cycle in the donor star.

For more information visit: http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006ApJ...636.1002S&db_key=AST&data_type=HTML&format=&high=42e557dd7e29466
Prepared By: Matthew Templeton
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