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Recent star formation history in the region of 30 Doradus

Published online by Cambridge University Press:  19 July 2016

M. -C. Lortet ,
G. Testor  and
N. Martin
M. -C. Lortet
Affiliation:
Observatoire de Meudon, F-92195 Meudon Cedex, France
G. Testor
Affiliation:
Observatoire de Meudon, F-92195 Meudon Cedex, France
N. Martin
Affiliation:
Observatoire de Marseille, F-13248 Marseille Cedex 04, France

Abstract

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The main purpose of our work is to study the range of ages of the stars in an area about 40' in diameter around R 136. Apart from individual stellar spectra, other age criteria may be found in photometric studies, the morphology and the density of the associated gas. In such complex regions as the 30 Dor region, estimating the depth along the line of sight is a problem.

Type
Star Formation and Clustering
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 155 - 156
Copyright
Copyright © Kluwer 1991 

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