Hydrogen and Helium Ionization in the Axisymmetric Envelopes of B[e] Supergiants

Details Hydrogen and Helium Ionization in the Axisymmetric Envelopes of B[e] Supergiants Hydrogen and Helium Ionization in the Axisymmetric Envelopes of B[e] Supergiants

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008rmxac..33...58z&link_type=abstract

Massive Stars: Fundamental Parameters and Circumstellar Interactions (Eds. P. Benaglia, G. L. Bosch, & C. E. Cappa) Revista Mexi

Astronomy and Astrophysics

Astronomy

Stars: Early-Type, Stars: Mass Loss

Scientific paper

Aims: Model atmospheres of B[e] supergiants (sgB[e]) were calculated to
test our newly developed 2D stellar atmosphere code (Astaroth). This
code will be used to study normal Be and sgB[e] stars, binaries with
colliding winds, LBVs, and type-II SNe. For simplicity, we included only
H, He, and C in the models presented here.

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