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Age of Luminous Blue Variable candidates from their stellar and nebular environment
Published online by Cambridge University Press: 12 April 2016
Abstract
The study of the context of LBV stars, that is close neighbourhood (companions) and spatial relationship to young objects such as cepheids. stellar associations, red supergiants. enriched OB supergiants. Hll regions. WR stars can provide useful clues on their true luminosity, their age thus eventually initial mass and evolutionary status.
- Type
- Section I: Main Papers, General Discussions, and Two Panel Discussions
- Information
- International Astronomical Union Colloquium , Volume 113: Physics of Luminous Blue Variables , 1989 , pp. 45 - 50
- Copyright
- Copyright © Kluwer 1989
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