2009MNRAS.394.2065K

Krtička J., Kubát J., 2009, "NLTE models of line-driven stellar winds III. Influence of X-ray radiation on wind structure of O stars", Mon. Not. R. Astron. Soc. 394, 2065 - 2079

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• some citations:
2009:
1. Marcolino, W. L. F.; Bouret, J. -C.; Martins, F.; Hillier, D. J.; Lanz, T.; Escolano, C.; 2009, "Analysis of Galactic late-type O dwarfs: more constraints on the weak wind problem", Astron. Astrophys. 498, 837 - 852

2010:
2. Sundqvist, J. O.; Puls, J.; Feldmeier, A.; 2010, "Mass loss from inhomogeneous hot star winds. I. Resonance line formation in 2D models", Astron. Astrophys. 510, A11
3. Waldron, W. L.; Cassinelli, J. P. 2010, "The Importance of XUV Radiation as a Solution to the P V Mass Loss Rate Discrepancy in O Stars", Astrophys. J. 711, L30 - L34
4. Cohen, D. H.; Leutenegger, M. A.; Wollman, E. E.; Zsargó, J.; Hillier, D. J.; Townsend, R. H. D.; Owocki, S. P. 2010, "A mass-loss rate determination for ζ Puppis from the quantitative analysis of X-ray emission-line profiles", Mon. Not. R. Astron. Soc. 405, 2391 - 2405

2011:
5. Sundqvist, J. O.; Puls, J.; Feldmeier, A.; Owocki, S. P., 2011, "Mass loss from inhomogeneous hot star winds II. Constraints from a combined optical/UV study", Astron. Astrophys. 528, A64
6. Kholtygin, A. F.; Sudnik, N. P.; Burlakova, T. E.; Valyavin, G. G. 2011, "Line-profile microvariability in OB-star spectra: the Supergiant λ Cep (O6If(n))", Astron. Rep. 55, 1105 - 1114
7. Puls, J.; 2011, "Winds from massive stars", Mem. Soc. Astron. It. 82, 774

2012:
8. Bouret, J.-C.; Hillier, D. J.; Lanz, T.; Fullerton, A. W., 2012, "Properties of Galactic early-type O-supergiants. A combined FUV-UV and optical analysis", Astron. Astrophys. 544, A67
9. Puebla, R. E.; Hillier, D. J.; Zsargó, J.; Cohen, D. H.; Leutenegger, M. A., 2016, "X-ray, UV and optical analysis of supergiants: ɛ Ori", Mon. Not. Roy. Astron. Soc. 456, 2907 - 2936


• autocitations:
2009:
• Krtička, J.; Feldmeier, A.; Oskinova, L. M.; Kubát, J.; Hamann, W.-R.; 2009, "X-ray emission from hydrodynamical simulations in non-LTE wind models", Astron. Astrophys. 508, 841 - 848
  
  2010:
• Krtička, J.; Kubát, J.; 2010, "Comoving frame models of hot star winds. I. Test of the Sobolev approximation in the case of pure line transitions", Astron. Astrophys. 519, A50
• Krtička, J.; Kubát, J.; 2010, "NLTE wind models of hot subdwarf stars", Astrophys. Space Sci. 329, 145 - 150

2012:
• Šurlan, B.; Hamann, W.-R.; Kubát, J.; Oskinova, L. M.; Feldmeier, A., 2012, "Three-dimensional radiative transfer in clumped hot star winds. I. Influence of clumping on the resonance line formation", Astron. Astrophys. 541, A37
• Krtička J., Kubát J., Skalický J., 2012, "X-Ray Photoionized Bubble in the Wind of Vela X-1 Pulsar Supergiant Companion", Astrophys. J. 757, 162
• Krtička J., Kubát J., 2012, "Influence of extreme ultraviolet radiation on the P V ionization fraction in hot star wind", Mon. Not. Roy. Astron. Soc. 427, 84 - 90

2014:
• Krtička J., 2014, "Mass loss in main-sequence B stars", Astron. Astrophys. 564, A70

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