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Near Infrared Observations of Magellanic WN Stars

Published online by Cambridge University Press:  14 August 2015

Y. Andrillat ,
M. Dennefeld  and
J.M. Vreux
Y. Andrillat
Affiliation:
Observatoire de Haute Provence, France
M. Dennefeld
Affiliation:
Institut d'Astrophysique, Paris, France
J.M. Vreux
Affiliation:
Institut d'Astrophysique, Liège, Belgium

Extract

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November 27, 1980, we had the opportunity to make near infrared observations of a few WR stars of the Magellanic Clouds with the ESO reticon system attached to the Boller and Chivens spectrograph at the 3.6 m telescope. The observing conditions as well as the reduction procedure have been described in another paper of this symposium (Vreux et al., 1982). We will immediately show how the near infra-red can be useful to improve our knowledge of some WR stars.

Type
SESSION 7 — WOLF-RAYET STARS IN EXTERNAL GALAXIES
Information
Symposium - International Astronomical Union , Volume 99: Wolf-Rayet Stars: Observations, Physics, Evolution , 1982 , pp. 527 - 530
Copyright
Copyright © Reidel 1982 

References

Allen, D.A. and Glass, I.S.: 1976, Astrophys. J. 210, 666.CrossRefGoogle Scholar
Andrillat, Y.: 1973, Mém. Soc. Roy. Sci. Liège sér. VI 5, 371.Google Scholar
Breysacher, J. and Westerlund, B.E.:1978, Astron. Astrophys. 67, 261.Google Scholar
Breysacher, J. and Perrier, C.: 1980, Astron. Astrophys. 90, 207.Google Scholar
Vreux, J.M., Dennefeld, M. and Andrillat, Y.: 1982, this symposium.Google Scholar
Walborn, N.R.: 1977, Astrophys. J. 215, 53.Google Scholar