Properties of Regions Forming the FeII Emission Lines in Be Stars

Thumbnail Image

Date

Authors

Journal Title

Journal ISSN

Volume Title

Publisher

Abstract

Description

We study FeII and Balmer hydrogen emission lines observed simultaneously of 18 southern Be stars. We use the self-absorption-curve method (SAC) to determine the optical depth regime of FeII emission lines and to derive first insights on the physical properties of their forming regions.
Societe Francaise d'Astronomie et d'Astrophysique, France (2005)

Keywords

Astrophysics

Citation

URI

https://dspace.dare.co.zw/handle/123456789/10405

Collections

arXiv

Endorsement

Review

Supplemented By

Referenced By