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Some Photometric Peculiarities of Symbiotic Stars
Published online by Cambridge University Press: 14 August 2015
Abstract
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The results of UBV photoelectric observations of 12 symbiotic stars have been considered. It must be noted that their light-curves are very different (irregular, regular, of Mira Ceti type) and, in the two-colour diagram (B – V)–(U – B), all these stars are located rather far to the right from the main sequence. The photometric peculiarities of symbiotic stars just mentioned can be explained by assuming that they are binary systems.
- Type
- Part 8 / Symbiotic Stars
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- Copyright
- Copyright © Reidel 1975
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