Quantitative Spectroscopy of the Brightest Blue Supergiant Stars in Galaxies
Abstract
Introduction Atmospheres of luminous hot stars Methods of spectral diagnostics The X-ray emission of O-stars IR - diagnostics of blue supergiants with extreme mass-loss The most massive stars in the Local Group Stellar abundances in Local Group galaxies and beyond The Wind Momentum - Luminosity Relationship and extragalactic distances Extragalactic stellar astronomy - a vision Appendix A. Oscillator strengths distribution function of hydrogen Reference
- Publication:
-
Stellar astrophysics for the local group: VIII Canary Islands Winter School of Astrophysics
- Pub Date:
- 1998
- Bibcode:
- 1998salg.conf..149K