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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

M.-C. Lortet
M.-C. Lortet*
Affiliation:
Département d’Astronomie extragalactique et de CosmologieObservatoire de ParisF-92195 Meudon Principal Cedex. France

Abstract

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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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