Number of the records: 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 - Journal Article
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
R&D Projects: GA ČR GA205/08/0003; GA ČR GD205/08/H005
Institutional research plan: CEZ:AV0Z10030501
Keywords : stars * outflows * mass-loss
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
Impact factor: 5.084, year: 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.
Permanent Link: http://hdl.handle.net/11104/0217372
Number of the records: 1