Article contents
Near Infrared Observations of Magellanic WN Stars
Published online by Cambridge University Press: 14 August 2015
Extract
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
- Copyright
- Copyright © Reidel 1982
References
- 2
- Cited by