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Age Determination of HII Regions of the LMC and SMC

Published online by Cambridge University Press:  04 August 2017

M. V. Copetti ,
H. A. Dottori ,
E. L. Bica  and
M. G. Pastoriza
M. V. Copetti
Affiliation:
Departamento de Astronomia, Instituto de Física, UFRGS and CNPq, BRAZIL
H. A. Dottori
Affiliation:
Departamento de Astronomia, Instituto de Física, UFRGS and CNPq, BRAZIL
E. L. Bica
Affiliation:
Departamento de Astronomia, Instituto de Física, UFRGS and CNPq, BRAZIL
M. G. Pastoriza
Affiliation:
Departamento de Astronomia, Instituto de Física, UFRGS and CNPq, BRAZIL

Abstract

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HII region models were constructed which take into account: ) A burst for the formation of the ionizing association; ) Different Salpeter's initial mass function () and upper stellar mass limit Models of stellar evolution with and without mass loss (Maeder, 1980, Hellings et al. 1981).

Type
Interstellar Matter
Information
Symposium - International Astronomical Union , Volume 108: Structure and Evolution of the Magellanic Clouds , 1984 , pp. 383 - 384
Copyright
Copyright © Reidel 1984 

References

Dottori, H.A.; Bica, E.L.D., 1981, Astron. Astrophys. 102, 245.Google Scholar
Dufour, R.J., 1975, Astrophys. J. 195, 315.CrossRefGoogle Scholar
Dufour, R.J.; Harlow, W.V., 1977, Astrophys. J. 216, 706.CrossRefGoogle Scholar
Hellings, P.; Vanbeveren, D., 1981, Astron. Astrophys. 95, 14.Google Scholar
Maeder, A., 1980, Astron. Astrophys. 92, 101.Google Scholar