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Absolute Magnitudes of Wolf-Rayet Stars: The WN3 and WN4 Sub-Classes in the Large Magellanic Cloud

Published online by Cambridge University Press:  14 August 2015

Jacques Breysacher  and
Marc Azzopardi
Jacques Breysacher
Affiliation:
European Southern Observatory, Karl Schwarzschild Strasse 2, D-8046 Garching bei München
Marc Azzopardi
Affiliation:
Observatoires du Pic-du-Midi et de Toulouse 1, av. C. Flammarion, F-31500 Toulouse

Extract

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After the systematic survey carried out by Azzopardi and Breysacher (1979, 1980) at La Silla, Chile, with the 40-cm Objective Prism Astrograph, the census of the Wolf-Rayet population (101 stars) in the Large Magellanic Cloud (LMC) can probably be considered as quite complete except, perhaps, for stars located in the core of dense HII regions. The catalogue by Breysacher (1981) includes 100 stars to which one has to add one star of the WN type discovered by Sanduleak (private communication) outside of the survey limits.

Type
SESSION 7 — WOLF-RAYET STARS IN EXTERNAL GALAXIES
Information
Symposium - International Astronomical Union , Volume 99: Wolf-Rayet Stars: Observations, Physics, Evolution , 1982 , pp. 523 - 526
Copyright
Copyright © Reidel 1982 

References

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