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Age of Luminous Blue Variable Candidates from their Stellar and Nebular Environment

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Physics of Luminous Blue Variables

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 157))

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, Hil regions. WR stars can provide useful clues on their true luminosity, their age thus eventually initial mass and evolutionary status.

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Author information

Authors and Affiliations

  1. Département d’Astronomie extragalactique et de Cosmologie, Observatoire de Paris, Meudon Primncipal Cedex, F-92195, France

    M.-C. Lortet

Authors
  1. M.-C. Lortet
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Editor information

Editors and Affiliations

  1. Department of Astronomy, University of Minnesota, Minneapolis, USA

    Kris Davidson

  2. Département de Physique, Université de Montréal, Canada

    A. F. J. Moffat

  3. SRON, Laboratory for Space Research, Utrecht, The Netherlands

    H. J. G. L. M. Lamers

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© 1989 Kluwer Academic Publishers

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Lortet, MC. (1989). Age of Luminous Blue Variable Candidates from their Stellar and Nebular Environment. In: Davidson, K., Moffat, A.F.J., Lamers, H.J.G.L.M. (eds) Physics of Luminous Blue Variables. Astrophysics and Space Science Library, vol 157. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-1031-7_5

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  • DOI: https://doi.org/10.1007/978-94-009-1031-7_5

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-6955-7

  • Online ISBN: 978-94-009-1031-7

  • eBook Packages: Springer Book Archive

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