| Body na spoluautora | Body za publikaci pro MU | Odkaz ISVaV | | 13,50 | 53,99 | The nature of the light variability of the silicon star HR 7224
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| 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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| 13,50 | 53,99 | The puzzling binary HD 143418
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| 2,24 | 6,72 | Advanced test of the model stellar atmospheres: the nature of the light variability of magnetic chemically peculiar 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 | Influence of the Frictional Heating on the Wind Line-Profiles of SMC Stars
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| 0,00 | 0,00 | The influence of clumping on predicted O star wind parameters
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| 2,24 | 4,48 | The influence of inhomogeneities on hot star wind model predictions
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| 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
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| 0,00 | 0,00 | Stellar winds and the circumstellar environment of massive first stars
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| 0,00 | 0,00 | The Nature of Light Variations of the He-Strong CP Star HD 37776
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| 0,00 | 0,00 | Light variations and angular momentum loss from the He-strong magnetic chemically peculiar star HD 37776
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| 3,36 | 6,72 | Mass-Loss and Multicomponent Flow from Central Stars of Planetary Nebulae
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| 0,00 | 0,00 | Multicomponent stellar winds and chemical peculiarity in A stars
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| 0,00 | 0,00 | NLTE wind models of A supergiants
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| 1,34 | 6,72 | Light variations and angular momentum loss from the He-strong magnetic chemically peculiar star HD 37776
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| 1,68 | 6,72 | The Nature of Light Variations of the He-Strong CP Star HD 37776
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| 0,00 | 0,00 | The dependence of the energy distribution on the abundances of A-star atmosphere models
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| 0,00 | 0,00 | The mass loss from hot Pop III stars
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| 2,24 | 4,48 | Mass Loss from Massive Zero-Metallicity Stars
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| 68,88 | 68,88 | NLTE models of line-driven stellar winds II. O stars in the Small Magellanic Cloud
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| 6,72 | 6,72 | NLTE wind models for SMC stars
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| 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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| 0,00 | 0,00 | The nature of the light variations of chemically peculiar stars
|
| 0,00 | 0,00 | Multicomponent stellar winds of B stars
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| 1,87 | 9,36 | mCP stars with photometrically simple behaviour
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| 2,24 | 4,48 | The mass loss from hot Pop III 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 | Rotational periods of magnetic chemically peculiar stars
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| 0,00 | 0,00 | Rotationally modulated photometric variations of mCP stars -- theoretical aspects
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| 1,17 | 9,36 | The record-breaking rotational deceleration of the He strong CP star HD 37776 (V901 Ori)
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| 0,00 | 0,00 | Wind emission of OB supergiants and the influence of clumping
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| 17,60 | 35,20 | Hot star wind models with new solar abundances
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| 4,92 | 49,23 | The extremely rapid rotational braking of the magnetic helium-strong star HD 37776
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| 0,00 | 0,00 | The extremely rapid rotational braking of the magnetic helium-strong star HD 37776
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| 0,00 | 0,00 | CNO driven winds of hot first stars
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| 0,00 | 0,00 | Chemicky pekuliární hvězdy - zmalované slečny
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| 18,00 | 35,99 | CNO-driven winds of hot first stars
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| 0,00 | 0,00 | The light variations of HD 37776 as a result of the uneven surface distribution of helium and silicon
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| 26,40 | 52,80 | The light variability of the helium strong star HD 37776 as a result of its inhomogeneous elemental surface distribution
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| 2,24 | 4,48 | Radiatively Driven Winds of OB Stars - from Micro to Macro
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| 0,00 | 0,00 | The ZOO of uvby and Hp light curves of magnetic chemically peculiar stars
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(c) Michal Bulant, 2011