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- Title
SIMECA: A CODE DEDICATED TO ACTIVE HOT STARS.
- Authors
Stee, Ph.; Meilland, A.; Kanaan, S.
- Abstract
Active hot stars are hot stars (Teff ≥ 8000 K) exhibiting emission lines (namely hydrogen lines) and IR excess which both originate in a circumstellar environment. In this paper we present in details the SIMECA (SImulation pour Etoiles Chaudes Actives) code which is the only code freely available to model the gaseous environment of active hot stars. It computes line profiles, Spectral Energy Distributions (SED) and intensity maps, which can be directly compared to high angular resolution observations.
- Subjects
EARLY stars; CIRCUMSTELLAR matter; SPECTRAL energy distribution; SPECTRUM analysis; QUASIELASTIC light scattering; SOLAR oscillations; STELLAR spectra; HIGH resolution spectroscopy; STARS
- Publication
EAS Publications Series, 2008, Vol 28, p135
- ISSN
1633-4760
- Publication type
Article
- DOI
10.1051/eas:0828019