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Wolf-Rayet Stars Associated to Giant Regions of Star Formation
Published online by Cambridge University Press: 14 August 2015
Abstract
Data on Wolf-Rayet (WR) stars in extragalactic H II regions and emission line galaxies are presented and discussed. The sample is still limited and inhomogeneous but two important points appear to be already established: a) The WR stars are more numerous than the blue supergiants at least in same phase of the evolution of the stellar clusters which ionize the giant H II regions, b) when the WR stars are detected, two cases are apparently observed, one in which only WN, the other in which both WN and WC, are present.
- Type
- SESSION 7 — WOLF-RAYET STARS IN EXTERNAL GALAXIES
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- Copyright © Reidel 1982