Radiatively Driven Winds of OB Stars - from Micro to Macro

Investor logo
Investor logo

Warning

This publication doesn't include Faculty of Arts. It includes Faculty of Science. Official publication website can be found on muni.cz.
Title in English Radiatively Driven Winds of OB Stars -- from Micro to Macro
Authors

KRTIČKA Jiří KUBÁT Jiří

Year of publication 2007
Type Article in Proceedings
Conference Active OB-Stars: Laboratories For Stellar and Circumstellar Physics
MU Faculty or unit

Faculty of Science

Citation
Web http://www.aspbooks.org/custom/publications/paper/index.phtml?paper_id=3935
Field Astronomy and astrophysics
Keywords stars: winds; stars:outflows; stars: mass-loss; stars: early-type
Description We review basic physics of line-driven stellar winds of OB stars. We discuss elementary processes due to which stellar winds are accelerated on a microscopic level. We show how these microscopic processes may enable the outflow and how they determine wind properties on a macroscopic level. We discuss shortcomings of present wind theories and future wind model improvements.
Related projects:

You are running an old browser version. We recommend updating your browser to its latest version.