Crossref Citations
This article has been cited by the following publications. This list is generated based on data provided by Crossref.
Krtička, J.
and
Kubát, J.
2004.
NLTE models of line-driven stellar winds.
Astronomy & Astrophysics,
Vol. 417,
Issue. 3,
p.
1003.
Proctor, M R E
2004.
Solar convection and magnetic fields.
Astronomy and Geophysics,
Vol. 45,
Issue. 4,
p.
4.14.
Low, B. C.
and
Zhang, M.
2004.
Magnetostatic Structures of the Solar Corona. III. Normal and Inverse Quiescent Prominences.
The Astrophysical Journal,
Vol. 609,
Issue. 2,
p.
1098.
Tobias, Steven
and
Weiss, Nigel
2004.
The puzzling structure of a sunspot.
Astronomy and Geophysics,
Vol. 45,
Issue. 4,
p.
4.28.
Sembach, K. R.
Wakker, B. P.
Tripp, T. M.
Richter, P.
Kruk, J. W.
Blair, W. P.
Moos, H. W.
Savage, B. D.
Shull, J. M.
York, D. G.
Sonneborn, G.
Hebrard, G.
Ferlet, R.
Vidal‐Madjar, A.
Friedman, S. D.
and
Jenkins, E. B.
2004.
The Deuterium‐to‐Hydrogen Ratio in a Low‐Metallicity Cloud Falling onto the Milky Way.
The Astrophysical Journal Supplement Series,
Vol. 150,
Issue. 2,
p.
387.
Kubát, Jiřı́
Krtička, Jiřı́
and
Pustylnik, Izold B.
2004.
Radiation induced coronal wind in late B stars.
New Astronomy,
Vol. 9,
Issue. 3,
p.
215.
Barklem, P. S.
2007.
Non-LTE Balmer line formation in late-type spectra: effects of atomic processes involving hydrogen atoms.
Astronomy & Astrophysics,
Vol. 466,
Issue. 1,
p.
327.
Romanyuk, I. I.
2007.
Main-sequence magnetic CP stars: II. Physical parameters and chemical composition of the atmosphere.
Astrophysical Bulletin,
Vol. 62,
Issue. 1,
p.
62.
Mashonkina, L.
Zhao, G.
Gehren, T.
Aoki, W.
Bergemann, M.
Noguchi, K.
Shi, J. R.
Takada-Hidai, M.
and
Zhang, H. W.
2008.
Non-LTE line formation for heavy elements in four very metal-poor stars.
Astronomy & Astrophysics,
Vol. 478,
Issue. 2,
p.
529.
Tycner, C.
Jones, C. E.
Sigut, T. A. A.
Schmitt, H. R.
Benson, J. A.
Hutter, D. J.
and
Zavala, R. T.
2008.
Constraining the Physical Parameters of the Circumstellar Disk of χ Ophiuchi.
The Astrophysical Journal,
Vol. 689,
Issue. 1,
p.
461.
Lind, K.
Korn, A. J.
Barklem, P. S.
and
Grundahl, F.
2008.
Atomic diffusion and mixing in old stars.
Astronomy & Astrophysics,
Vol. 490,
Issue. 2,
p.
777.
Jones, C. E.
Tycner, C.
Sigut, T. A. A.
Benson, J. A.
and
Hutter, D. J.
2008.
A Parameter Study of Classical Be Star Disk Models Constrained by Optical Interferometry.
The Astrophysical Journal,
Vol. 687,
Issue. 1,
p.
598.
Önehag, A.
Gustafsson, B.
Eriksson, K.
and
Edvardsson, B.
2009.
Calibration of Strömgrenuvby-Hβphotometry for late-type stars – a model atmosphere approach.
Astronomy & Astrophysics,
Vol. 498,
Issue. 2,
p.
527.
Šurlan, Brankica
and
Kubát, Jiří
2010.
Line profiles of OB star winds using a Monte Carlo method.
Proceedings of the International Astronomical Union,
Vol. 6,
Issue. S272,
p.
214.
Krtička, Jiří
and
Kubát, Jiří
2010.
NLTE wind models of hot subdwarf stars.
Astrophysics and Space Science,
Vol. 329,
Issue. 1-2,
p.
145.
Kubát, Jiří
and
Šurlan, Brankica
2014.
Determination of Atmospheric Parameters of B-, A-, F- and G-Type Stars.
p.
159.
Cortés, C.
Maciel, S. C.
Vieira, S.
Ferreira Lopes, C. E.
Leão, I. C.
de Oliveira, G. P.
Correia, C.
Canto Martins, B. L.
Catelan, M.
and
De Medeiros, J. R.
2015.
Stellar parameters for stars of the CoRoT exoplanet field.
Astronomy & Astrophysics,
Vol. 581,
Issue. ,
p.
A68.