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On the Detection of WR Stars in Nearby Galaxies

Published online by Cambridge University Press:  03 August 2017

J. Lequeux  and
M. Azzopardi
J. Lequeux
Affiliation:
Observatoire de Meudon 91195 Meudon CEDEX, France and Ecole Normale Supérieure
M. Azzopardi
Affiliation:
Observatoire de Marseille 13248 Marseille CEDEX, France

Abstract

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The different methods for detecting WR stars in nearby galaxies are reviewed and compared. Each one has its own advantages and drawbacks, and they are complementary rather than competing. Both monochromatic filter imaging and field- or single-object spectroscopy are required for an absolutely safe detection of objects near the limit. The results obtained to-date are shortly reviewed and perspectives are discussed.

Type
Session VIII. Inventory and Distribution
Information
Symposium - International Astronomical Union , Volume 143: Wolf–Rayet Stars and Interrelations with other Massive Stars in Galaxies , 1991 , pp. 619 - 624
Copyright
Copyright © Kluwer 1991 

References

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