No CrossRef data available.
Article contents
New analysis of Wolf-Rayet infrared lines
Published online by Cambridge University Press: 07 August 2017
Abstract
New infrared spectra of Wolf-Rayet stars are analysed to derive C/He abundance ratios and ionization ratios. These ratios are discussed in relation with subtype, terminal velocity and local metallicity. They are compared with the predictions of evolutionary models.
- Type
- Session II - Model atmospheres for single Wolf-Rayet stars
- Information
- Copyright
- Copyright © Kluwer 1995