Body na spoluautora | Body za publikaci pro MU | Odkaz ISVaV | 28,23 | 56,45 | NLTE models of line-driven stellar winds III. Influence of X-ray radiation on wind structure of O stars
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27,00 | 53,99 | X-ray emission from hydrodynamical simulations in non-LTE wind models
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0,00 | 0,00 | Challenges to the theories of B stars circumstellar environment
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17,60 | 35,20 | The winds of hot massive first stars
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0,00 | 0,00 | The influence of clumping on predicted O star wind parameters
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0,00 | 0,00 | Influence of the Frictional Heating on the Wind Line-Profiles of SMC Stars
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2,24 | 4,48 | The influence of inhomogeneities on hot star wind model predictions
|
0,00 | 0,00 | The Influence of X-ray Emission on the Stellar Wind of O Stars
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0,00 | 0,00 | Synthetic spectra of A supergiants
|
0,00 | 0,00 | Stellar winds and the circumstellar environment of massive first stars
|
3,36 | 6,72 | Mass-Loss and Multicomponent Flow from Central Stars of Planetary Nebulae
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0,00 | 0,00 | NLTE wind models of A supergiants
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0,00 | 0,00 | Multicomponent stellar winds and chemical peculiarity in A stars
|
0,00 | 0,00 | Spectroscopic and Photometric Observations of SN 2004dj
|
2,24 | 4,48 | Mass Loss from Massive Zero-Metallicity Stars
|
0,00 | 0,00 | The mass loss from hot Pop III stars
|
17,60 | 35,20 | Multicomponent radiatively driven stellar winds IV. On the helium decoupling in the wind of sigma Ori E
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2,24 | 4,48 | The mass loss from hot Pop III stars
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0,00 | 0,00 | Multicomponent stellar winds of B stars
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0,00 | 0,00 | Stationary Model of a Line Driven Wind with Rotation
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0,00 | 0,00 | Wind emission of OB supergiants and the influence of clumping
|
17,60 | 35,20 | Hot star wind models with new solar abundances
|
18,00 | 35,99 | CNO-driven winds of hot first stars
|
0,00 | 0,00 | CNO driven winds of hot first stars
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2,24 | 4,48 | Radiatively Driven Winds of OB Stars - from Micro to Macro
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(c) Michal Bulant, 2011