Abstract
A method is suggested for using the measured frequency dependent diameters to test the atmospheric structure of late-type supergiants. The efficiency of the methodvis-à-vis limb-darkening measurements is discussed.
References
Böhm, K. H.: 1961,Astrophys. J. 134, 264.
Bonneau, D. and Labeyrie, A.: 1973,Astrophys. J. (Letters) 181, L1.
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On leave from the Tata Institute of Fundamental Research, Bombay, India.
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Vardya, M.S. Frequency dependent diameters and atmospheric structure of late-type supergiants. Astrophys Space Sci 47, L15–L16 (1977). https://doi.org/10.1007/BF00651377
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DOI: https://doi.org/10.1007/BF00651377