H(alpha) Emission from Late Type Be Stars

Details H(alpha) Emission from Late Type Be Stars H(alpha) Emission from Late Type Be Stars

Sep 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997japa...18..145a&link_type=abstract

Journal of Astrophysics and Astronomy, Vol. 18, p.145

Astronomy and Astrophysics

Astrophysics

2

Be Stars, H-Alpha Line, He Stars

Scientific paper

We show here that the H(alpha) flux from late type Be stars can be
explained as emission from an HII regions formed in the gas envelope
around the Be star, by the UV flux emitted by a helium star binary
companion. We also discuss the observability of the helium star
companions.

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