2001A&A...369..222K
Krtička J., Kubát J., 2001,
"Multicomponent radiatively driven stellar winds I. Nonisothermal
three-component wind of hot B stars",
Astron. Astrophys. 369, 222 - 238
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postscript
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- some citations:
2002:
-
Owocki S. P., Puls J., 2002,
"Ion runaway instability in low-density, line-driven stellar
winds",
Astrophys. J. 568, 965 - 978
-
Kudritzki, R.-P., 2002,
"Line-driven Winds, Ionizing Fluxes, and Ultraviolet Spectra of Hot
Stars at Extremely Low Metallicity. I. Very Massive O Stars",
Astrophys. J. 577, 389 - 408
2003:
-
Groote D., 2003,
"Relationship between surface and wind abundances in Bp stars",
in International conference on magnetic fields in O, B, and A stars,
L. A. Balona, H. F. Henrichs & T. Medupe eds., ASP Conf. Ser. Vol.
305, p. 243 - 251
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Owocki S., ud-Doula A., 2003,
"Magnetic spin-up of line driven stellar winds",
in International conference on magnetic fields in O, B, and A stars,
L. A. Balona, H. F. Henrichs & T. Medupe eds., ASP Conf. Ser. Vol.
305, p. 350 - 357
2004:
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Groote D., Schmitt J. H. M. M., 2004,
"Discovery of X-ray flaring on the magnetic Bp-star
σ Ori E",
Astron. Astrophys. 418, 235 - 242
2007:
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Owocki, S. P. 2007,
"Overview of Active OB Stars:,
in Active OB-Stars: Laboratories for Stellar and Circumstellar Physics,
S. Štefl, S. P. Owocki, & A. T. Okazaki eds., ASP Conf. Ser. Vol. 361,
p. 3 - 14
2008:
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Martins, F.; Gillessen, S.; Eisenhauer, F.; Genzel, R.; Ott, T.; Trippe, S.
2008,
"On the Nature of the Fast-Moving Star S2 in the Galactic Center",
Astrophys. J. 672, L119 - L122
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Unglaub, K. 2008,
"Mass-loss and diffusion in subdwarf B stars and hot white dwarfs: do
weak winds exist?",
Astron. Astrophys. 486, 923 - 940
2009:
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Cranmer, S. R.
2009,
"A Pulsational Mechanism for Producing Keplerian Disks Around Be
Stars",
Astrophys. J. 701, 396 - 413
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Puls, J.; Sundqvist, J. O.; Najarro, F.; Hanson, M. M.; 2009,
"Mass loss from OB-stars",
in Recent Directions in Astrophysical Quantitative Spectroscopy and
Radiation Hydrodynamics,
AIP Conf. Proc. Vol. 1171, p. 123 - 135
2010:
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Jeffery, C. S.; Hamann, W.-R.; 2010,
"Stellar winds and mass loss from extreme helium stars",
Mon. Not. R. Astron. Soc 404, 1698 - 1710
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Hamann, W.-R. 2010,
"Stellar winds from hot low-mass stars",
Astrophys. Space Sci. 329, 151 - 158
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Staritsin, E. I. 2010,
"Upper limit for the mass loss rate of rapidly rotating single
main-sequence O9-B4 stars",
Astron. Lett. 36, 796 - 807
2011:
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Zboril, M. 2011,
"Properties of He-rich stars. IV. Search for He vertical
stratification",
Astrophys. Space Sci. 332, 163 - 170
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Puls, J.; 2011,
"Winds from massive stars",
Mem. Soc. Astron. It. 82, 774
2014:
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Staritsin, E. I., 2014,
"Enhancement of surface helium abundance in intermediate-mass
main-sequence stars",
Astron. Rep. 58, 808 - 824
- weak autocitations:
2011:
- Mikulášek, Z.; Krtička, J.; Henry, G. W.; Janík, J.; Zverko, J.;
Žižňovský, J.; Zejda, M.; Liška, J.; Zvěřina, P.; Kudrjavtsev, D. O.;
Romanyuk, I. I.; Sokolov, N. A.; Lüftinger, T.; Trigilio, C.; Neiner,
C.; de Villiers, S. N. 2011,
"Surprising variations in the rotation of the chemically peculiar
stars CU Virginis and V901 Orionis",
Astron. Astrophys. 534, L5
- some autocitations:
2001:
- Krtička J., Kubát J., 2001,
"Multicomponent radiatively driven stellar winds II. Gayley-Owocki
heating in multitemperature winds of OB stars",
Astron. Astrophys. 377, 175 - 191
2002:
- Krtička J., Kubát J., 2002,
"Multicomponent radiatively driven stellar winds III.
Radiative-acoustic waves in a two-component wind",
Astron. Astrophys. 388, 531 - 539
2003:
-
Krtička, J., 2003,
"Modeling of Multicomponent Radiatively Driven Stellar Winds Using a
Newton-Raphson Method",
in Stellar Atmosphere Modelling, I. Hubeny, D. Mihalas & K. Werner
eds., ASP Conf. Ser., p. 259 - 262
2004:
-
Krtička J., Kubát J., 2004,
"Multicomponent stellar winds of He chemically peculiar stars",
in Magnetic stars, Yu. Glagolevskij, D. Kudryavtsev, & I. Romanyuk
eds., Nizhnij Arkhyz, p. 234 - 240
(astro-ph/0310751)
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
Last update 13.11.2014