PHOENIX Spectra of Red Supergiants - Varying the Surface Abundances and the Microturbulence

Details PHOENIX Spectra of Red Supergiants - Varying the Surface Abundances and the Microturbulence PHOENIX Spectra of Red Supergiants - Varying the Surface Abundances and the Microturbulence

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..425...61l&link_type=abstract

Hot and Cool: Bridging Gaps in Massive Star Evolution ASP Conference Series Vol. 425, Proceedings of a Workshop held at the Cali

Astronomy and Astrophysics

Astronomy

Scientific paper

Based on PHOENIX models, we briefly discuss effects of surface
abundances and microturbulence on the near-IR spectra of red supergiant
stars.

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