Herbig Ae/Be stars

被引：246

作者：

Waters, LBFM

Waelkens, C

机构：

[1] Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1098 SJ Amsterdam, Netherlands

[2] Katholieke Univ Leuven, Inst Sterrenkunde, B-3001 Heverlee, Belgium

来源：

ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS | 1998年 / 36卷

关键词：

pre-main-sequence stars; circumstellar matter; protoplanetary systems; stellar evolution;

D O I：

10.1146/annurev.astro.36.1.233

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 beta Pictoris is summarized.

引用

页码：233 / 266

页数：34

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