Počet záznamů: 1
3-D Monte Carlo Radiative Transfer Calculation of Resonance Line Formation in the Inhomogeneous Expanding Stellar Wind
- 1.0439741 - ASÚ 2015 RIV US eng C - Konferenční příspěvek (zahraniční konf.)
Šurlan, Brankica - Hamann, W.-R. - Kubát, Jiří - Oskinova, L.M. - Feldmeier, A.
3-D Monte Carlo Radiative Transfer Calculation of Resonance Line Formation in the Inhomogeneous Expanding Stellar Wind.
Four Decades of Research On Massive Stars. San Francisco: Astronomical Society of the Pacific, 2012 - (Drissen, L.), s. 134-139. ASP Conference Series, 465. ISBN 978-1-58381-812-1.
[Meeting on 4 Decades of Research on Massive Stars in Honor of Anthony FJ Moffat. Auberge Lac Taureau (CA), 11.07.2011-15.07.2011]
Institucionální podpora: RVO:67985815
Klíčová slova: bright ob-stars * mass-loss rates * zeta puppis
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika
We study the effects of optically thick clumps, non-void interclump medium, variation of the onset of clumping, and velocity dispersion inside clumps on the formation of resonance lines.
Trvalý link: http://hdl.handle.net/11104/0242949
Počet záznamů: 1