HERBIG Ae/Be STARS-Reference-Cited by-同舟云学术

HERBIG Ae/Be STARS

Published:1998-09 Issue:1 Volume:36 Page:233-266
ISSN:0066-4146
Container-title:Annual Review of Astronomy and Astrophysics
language:en
Short-container-title:Annu. Rev. Astron. Astrophys.

Author:

Waters L. B. F. M.¹,Waelkens C.²

Affiliation:

1. Astronomical Institute Anton Pannekoek, University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam;

2. Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestÿnen laan 200B, B-3001 Heverlee, Belgium;

Abstract

▪ Abstract We review the wide range of observed properties of Herbig Ae/Be stars and try to combine this rich data set into a consistent picture of their circumstellar environment and evolutionary status. We discuss in some detail the geometry of the circumstellar environment. The presence of disks in Herbig Ae/Be stars is inferred from direct and indirect observational evidence. Envelopes can dominate the spectral energy distributions on large angular scales. In some stars, a fairly massive disk persists until the star has reached the main sequence. The evidence for an evolutionary link between isolated Herbig Ae/Be stars and β Pictoris is summarized.

Publisher

Annual Reviews

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://www.annualreviews.org/doi/pdf/10.1146/annurev.astro.36.1.233

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