Počet záznamů: 1
Three-dimensional radiative transfer in clumped hot star winds I. Influence of clumping on the resonance line formation
- 1.0388468 - ASÚ 2013 RIV FR eng J - Článek v odborném periodiku
Šurlan, Brankica - Hamann, W.-R. - Kubát, Jiří - Oskinova, L.M. - Feldmeier, A.
Three-dimensional radiative transfer in clumped hot star winds I. Influence of clumping on the resonance line formation.
Astronomy & Astrophysics. Roč. 541, May (2012), A37/1-A37/11. ISSN 0004-6361. E-ISSN 1432-0746
Grant CEP: GA ČR GA205/08/0003; GA ČR GD205/08/H005
Výzkumný záměr: CEZ:AV0Z10030501
Klíčová slova: stars * outflows * mass-loss
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika
Impakt faktor: 5.084, rok: 2012
We incorporate the 3D nature of the stellar wind clumping into radiative transfer calculations and investigate how different model parameters influence the resonance line formation.
Trvalý link: http://hdl.handle.net/11104/0217372
Počet záznamů: 1