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The HR diagram of LMC supergiant stars

Published online by Cambridge University Press:  07 August 2017

A. Bressan ,
G. Bertelli  and
C. Chiosi
A. Bressan
Affiliation:
Department of Astronomy and Astronomical Observatory Vicolo dell'Osservatorio 5 35122 Padova Italy
G. Bertelli
Affiliation:
Department of Astronomy and Astronomical Observatory Vicolo dell'Osservatorio 5 35122 Padova Italy
C. Chiosi
Affiliation:
Department of Astronomy and Astronomical Observatory Vicolo dell'Osservatorio 5 35122 Padova Italy

Abstract

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We analyze the HR diagram of LMC supergiant stars using a new set of evolutionary models for massive stars.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 149: The Stellar populations of Galaxies , 1992 , pp. 396
Copyright
Copyright © Kluwer 

References

Alongi, M., Bertelli, G., Bressan, A., Chiosi, C., Fagotto, F., Greggio, L., Nasi, E., 1991a, A.&A. submitted.Google Scholar
Caughlan, G.R., Fowler, W.A., 1988, Atomic Data Nuc. Data Tables 40, 283.CrossRefGoogle Scholar
de Jager, C., Nieuwenhuijzen, H., van der Hucht, K.A., 1988 AAS 72, 259.Google Scholar
Fitzpatrick, E.L., Garmany, C.D., 1990, ApJ 363, 119.CrossRefGoogle Scholar
Iglesias, C.A., Rogers, FJ., Wilson, B.G., 1990, ApJ 360, 221.CrossRefGoogle Scholar
Langer, N., 1989, AA 210, 93.Google Scholar
Tuchman, J., Wheeler, J.C., 1990, ApJ 363, 255.CrossRefGoogle Scholar