New self-consistent wind parameters to fit optical spectra of O-type stars
Abstract
We perform spectral fittings for O-type stars based on self-consistent wind solutions, providing Ṁ and ν(r directly derived from the initial stellar parameters. We introduce our two methods: m-CAK prescription and Lambert-procedure.
- Publication:
-
IAU Symposium
- Pub Date:
- 2024
- DOI:
- 10.1017/S1743921322002605
- Bibcode:
- 2024IAUS..361..190G
- Keywords:
-
- Early-type stars;
- Hydrodynamics;
- Stellar winds