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New Models for Massive Star Populations in Young Starbursts: Summary of the Models and Applications
Published online by Cambridge University Press: 25 May 2016
Extract
Using the latest stellar evolution models, theoretical stellar spectra, and a compilation of observed emission line strengths from Wolf-Rayet (WR) stars, we have constructed evolutionary synthesis models for young starbursts (Schaerer & Vacca 1997; see also Schaerer 1996). We provide detailed predictions of UV and optical emission line strengths for both the WR stellar lines and the major nebular hydrogen and helium emission lines, as a function of several input parameters related to the starburst episode.
- Type
- Starbursts
- Information
- Copyright
- Copyright © Kluwer 1999