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Line profiles of OB star winds using a Monte Carlo method
- 1.0372635 - ASÚ 2012 RIV GB eng C - Conference Paper (international conference)
Šurlan, Brankica - Kubát, Jiří
Line profiles of OB star winds using a Monte Carlo method.
Active OB stars: structure, evolution, mass loss, and critical limits. Cambridge: Cambridge University Press, 2011 - (Neiner, C.), s. 214-215. IAU Symposium Proceedings Series, IAU S272. ISBN 978-0-521-19840-0. ISSN 1743-9213.
[Symposium of the International Astronomical Union /272./. Paris (FR), 19.07.2010-23.07.2010]
R&D Projects: GA ČR GA205/08/0003; GA ČR GD205/08/H005
Institutional research plan: CEZ:AV0Z10030501
Keywords : radiative transfer * stars winds * outflows
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
The solution of the radiative transfer in an expanding atmospheres using the Monte Carlo method is presented. We applied our method to winds of several OB stars. In our calculation, the velocity and density structure is assumed to be given. Selected line profiles are shown.
Permanent Link: http://hdl.handle.net/11104/0205900
Number of the records: 1