Hydrogen and helium ionization in the axisymmetric envelopes of B[e] supergiants

J. Zsargó, D. J. Hillier, L. N. Georgiev

Research output: Contribution to journalConference articlepeer-review

Abstract

Aims: Model atmospheres of B[e] supergiants (sgB[e]) were calculated to test our newly developed 2D stellar atmosphere code (As- taroth). 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.

Original languageEnglish
Pages (from-to)58
Number of pages1
JournalRevista Mexicana de Astronomia y Astrofisica: Serie de Conferencias
Volume33
StatePublished - 2008
Externally publishedYes
EventMassive Stars: Fundamental Parameters and Circumstellar Interactions - Carilo, Buenos Aires, Argentina
Duration: 11 Dec 200614 Dec 2006

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