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The envelopes of the Herbig Ae/Be stars

  • C. Catala
Part V: Stellar Content of Nearby Molecular Clouds
Part of the Lecture Notes in Physics book series (LNP, volume 237)

Abstract

First identified by Herbig (1960), the Herbig Ae/Be stars are usually considered as pre-main sequence objects of intermediate mass, and are found at the edges of regions of heavy obscuration.

The study of the interaction of these stars with their surrounding clouds is subordinated to a good knowledge of the structure of their envelopes. The present paper is devoted to a brief review of the observational data available for these stars, and of the constraints on the structure of their envelopes that can be derived from these data.

Keywords

Mass Loss Rate Molecular Cloud Monthly Notice Tauri Star Molecular Flow 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag 1985

Authors and Affiliations

  • C. Catala
    • 1
  1. 1.Observatoire de Paris-MeudonMeudon Principal CedexFrance

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