Properties of Regions Forming the FeII Emission Lines in Be Stars

Details Properties of Regions Forming the FeII Emission Lines in Be Stars Properties of Regions Forming the FeII Emission Lines in Be Stars

2005-09-07

arxiv.org/abs/astro-ph/0509178v1

Astronomy and Astrophysics

Astrophysics

Societe Francaise d'Astronomie et d'Astrophysique, France (2005)

Scientific paper

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.

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