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A Model for the Shell of HD 50138*
Published online by Cambridge University Press: 14 August 2015
Abstract
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A model for the shell star HD 50138 is inferred from the observation of the continuous spectrum from 0.14 to 10 μ.
- Type
- Part 1: Observations of Be Stars
- Information
- Copyright
- Copyright © Reidel 1976
References
Boksenberg, A., Evans, R. G., Fowler, R. G., Gardner, I. S. K., Houziaux, L., Humphries, C. M., Jamar, C., Macau, D., Malaise, D., Monfils, A., Nandy, K., Thompson, G. I., Wilson, R., and Wroe, H.: 1973,
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Kurucz, R. L., Peytremann, E., and Avrett, E. H.: 1974, Smithsonian Astrophysical Observatory, Washington D.C.
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Kurucz, R. L. and Peytremann, E.: 1975, Special Report, Smithsonian Astrophysical Observatory.Google Scholar
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