Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-25T22:41:45.337Z Has data issue: false hasContentIssue false
  • English
  • Français

Multicomponent stellar winds and chemical peculiarity in A stars

Published online by Cambridge University Press:  02 March 2005

Jiří Krtička  and
Jiří Kubát
Jiří Krtička
Affiliation:
Ústav teoretické fyziky a astrofyziky PřF, Masarykova univerzita, CZ-611 37 Brno, Czech Republic, email: [email protected]
Jiří Kubát
Affiliation:
Astronomický ústav, Akademie věd České republiky, CZ-251 65 Ondřejov, Czech Republic, email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We calculate multicomponent radiatively driven stellar wind models suitable for A stars. We discuss the possible decoupling of individual elements from the stellar wind and its influence on the chemical peculiarity of these stars. We obtain a range of stellar parameters for different types of multicomponent flow.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Hydrodynamicsstars: mass lossstars: early-typestars: winds
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS224 , July 2004 , pp. 201 - 207
Copyright
© 2004 International Astronomical Union