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The stellar content of NGC 2363 and its surroundings

Published online by Cambridge University Press:  25 May 2016

Laurent Drissen ,
Jean-René Roy ,
Carmelle Robert  and
Daniel Devost
Laurent Drissen
Affiliation:
Département de Physique and Observatoire du Mont Mégantic, Université Laval, Québec, Qc G1K 7P4, Canada
Jean-René Roy
Affiliation:
Département de Physique and Observatoire du Mont Mégantic, Université Laval, Québec, Qc G1K 7P4, Canada
Carmelle Robert
Affiliation:
Département de Physique and Observatoire du Mont Mégantic, Université Laval, Québec, Qc G1K 7P4, Canada
Daniel Devost
Affiliation:
Département de Physique and Observatoire du Mont Mégantic, Université Laval, Québec, Qc G1K 7P4, Canada

Abstract

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A detailed study of the stellar content of the giant H II region NGC 2363 and its surroundings in the Magellanic galaxy NGC 2366 is undertaken to understand the starburst phenomenon.

Type
Part 6. Starbursts in normal and active galaxies: their effects on the ISM and on chemical evolution
Information
Symposium - International Astronomical Union , Volume 193: Wolf-Rayet Phenomena in Massive Stars and Starburst Galaxies , 1999 , pp. 741 - 742
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Drissen, L., Roy, J.-R., Moffat, A.F.J. 1993, AJ 106, 1460 Google Scholar
Drissen, L., Roy, J.-R., Robert, C. 1997, ApJ 474, L35 Google Scholar
Roy, J.-R., Aubé, M., McCall, M.L., Dufour, R.J. 1992, ApJ 386, 498 Google Scholar