Abstract
The mass deduced, using photometrically determinedg, gives a lower limit to the mass. Furthermore, mass determination in giant and supergiant stars may be effected byg andT eff being determined for different values of the stellar radius.
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References
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On leave from the Tata Institute of Fundamental Research, Bombay, India.
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Vardya, M.S. On mass determination fromT eff,g, andM bol . Astrophys Space Sci 41, L1–L2 (1976). https://doi.org/10.1007/BF00684585
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DOI: https://doi.org/10.1007/BF00684585