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Statistical Analysis of the Data Available for Be Stars

Published online by Cambridge University Press:  14 August 2015

Daniel Egret
Daniel Egret*
Affiliation:
Observatoire de Strasbourg

Extract

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A comprehensive catalogue of more than 1100 Be stars with known MK classification has been prepared at the Strasbourg Stellar Data Center, and is described in an other session of this Symposium (Jaschek and Egret, 1982). The compilation of photometric and spectroscopic data available for these stars has made possible a general statistical approach of the Be star spectral group.

Type
I. Photometry
Information
Symposium - International Astronomical Union , Volume 98: Be Stars , 1982 , pp. 27 - 31
Copyright
Copyright © Reidel 1982 

References

Egret, D.: 1981, (in preparation).Google Scholar
Feinstein, A. and Maracco, H.J.: 1979, Astron. J. 84, 1713.Google Scholar
FitzGerald, P.: 1970, Astron. Astrophys. 4, 234.Google Scholar
Houk, N. and Cowley, A.P.: 1975, Michigan Catalogue of Two-dimensional Spectral Types for the HD Stars, vol. I, Michigan Univ. Google Scholar
Houk, N.: 1978, Michigan Catalogue of Two-dimensional Spectral Types for the HD Stars, vol. II, Michigan Univ. Google Scholar
Jaschek, M. and Egret, D.: 1982, IAU Symp. 98 “Be stars”, Jaschek, M. and Groth, H.G. eds., p. 261 Google Scholar
Nicolet, B.: 1978, Astron. Astrophys. Suppl. Ser. 34, 1.Google Scholar
Uesugi, A. and Fukuda, I.: 1981, Proc. of 7th International CODATA Conference (in press).Google Scholar