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Progress in model atmosphere studies of Wolf-Rayet stars
Published online by Cambridge University Press: 25 May 2016
Abstract
Recent progress in the quantitative analysis of Wolf-Rayet stars is reviewed, emphasising the role played by choice of spectral diagnostics, clumping and line-blanketing on derived stellar properties. The ionizing properties of WR stars are discussed, based on clumped, line-blanketed models for WN and WC stars. The role of metallicity and mass-loss is assessed, and the role of H II regions as probes of predicted Lyman continuum distributions. Suggestions are made for differences in observed properties of WCE and WO subtypes.
- Type
- Part 2. Models for single star evolution of massive stars: wind + atmosphere + interior
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- Copyright © Astronomical Society of the Pacific 1999