A Photometric Study of Selected Near-Contact Binary Systems
The light curves of 16 near-contact binaries (10 from published observations and 6 from our own observations) from the catalog by Shaw (1994) have been solved in a homogeneous manner in order to determine their subclass and to extract their absolute elements. The evolutionary state of the near-contact class of intaracting binaries as it is determined from these elements shows that in general these systems are more evolved than the W UMa type contact binaries.
KeywordsStars: eclipsing binaries: near-contact stars: photometry stars: evolution
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