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Some Properties of S Mira Variables

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Cool Stars with Excesses of Heavy Elements

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 114))

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Abstract

Some correlations between period of pulsation, spectral type at maximum, mean difference in visual magnitude between maxima and minima, intensity of Tc I line, ratio of the number of days from minimum to the next following maximum to the period, and infrared colour index [11μ] − [3.5 μ] are described for S Mira variables.

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© 1985 D. Reidel Publishing Company

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Vardya, M.S. (1985). Some Properties of S Mira Variables. In: Jaschek, M., Keenan, P.C. (eds) Cool Stars with Excesses of Heavy Elements. Astrophysics and Space Science Library, vol 114. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5325-3_14

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  • DOI: https://doi.org/10.1007/978-94-009-5325-3_14

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-8851-0

  • Online ISBN: 978-94-009-5325-3

  • eBook Packages: Springer Book Archive

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