2012A&A...541A..37S

Šurlan B., Hamann, W.-R., Kubát J., Oskinova L., 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

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• some citations:
2013:
1. Sundqvist J. O., Owocki S. P., 2013, "Clumping in the inner winds of hot, massive stars from hydrodynamical line-driven instability simulations", Mon. Not. Roy. Astron. Soc. 428, 1837 - 1844
2. Laursen P., Duval F., Östlin G., 2013, "On the (Non-)Enhancement of the Lyα Equivalent Width by a Multiphase Interstellar Medium", Astrophys. J. 766, 124,
3. Zhang Y., Hou S.-Q., Yang P., Wu K.-S., 2013, "High-Precision Direct Method for the Radiative Transfer Problems", Comm. Theor. Phys. 59, 782 - 788
4. Prinja, R. K.; Massa, D. L., 2013, "Ultraviolet diagnostic of porosity-free mass-loss estimates in B stars", Astron. Astrophys. 559, A15


2014:
5. Groh J. H., Meynet G., Ekström S., Georgy C., 2014, "The evolution of massive stars and their spectra. I. A non-rotating 60 M_⊙ star from the zero-age main sequence to the pre-supernova stage", Astron. Astrophys. 564, A30
6. Krtička J., 2014, "Mass loss in main-sequence B stars", Astron. Astrophys. 564, A70
7. Petrov B., Vink J. S., Gräfener G., 2014, "On the Hα behaviour of blue supergiants: rise and fall over the bi-stability jump", Astron. Astrophys. 565, A62
8. Sundqvist, J. O.; Puls, J.; Owocki, S. P., 2014, "Mass loss from inhomogeneous hot star winds. III. An effective-opacity formalism for line radiative transfer in accelerating, clumped two-component media, and first results on theory and diagnostics", Astron. Astrophys. 568, A59


2015:
9. Massa, D.; Prinja, R. K., 2015, "On the Origin of Wind Line Variability in O Stars", Astrophys. J. 809, 12
10. Noebauer, U. M.; Sim, S. A., 2015, "Self-consistent modelling of line-driven hot-star winds with Monte Carlo radiation hydrodynamics", Mon. Not. Roy. Astron. Soc. 453, 3120
2016:
11. 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


• weak autocitations:
2012:
1. Oskinova, L. M.; Feldmeier, A.; Kretschmar, P. 2012, "Clumped stellar winds in supergiant high-mass X-ray binaries: X-ray variability and photoionization", Mon. Not. Roy. Astron. Soc. 421, 2820 - 2831
2. Naze Y., Oskinova L. M., Gosset E., 2012, "A detailed X-ray investigation of zeta Puppis - The variability on short and long timescales", Astrophys. J., in press
2013:
3. Oskinova L. M., Sun W., Evans C. J., Hénault-Brunet V., Chu Y.-H., Gallagher J. S. III, Guerrero M. A., Gruendl R. A., Güdel M., Silich S., Chen Y., Nazé Y., Hainich R., Reyes-Iturbide J., 2013, "Discovery of X-Ray Emission from Young Suns in the Small Magellanic Cloud", Astrophys. J. 765, 73
4. Oskinova L. M., Guerrero M. A., Hénault-Brunet V., Sun W., Chu Y.-H., Evans C., Gallagher J. S., Gruendl R. A., Reyes-Iturbide J., 2013, "The slow X-ray pulsar SXP 1062 and associated supernova remnant in the Wing of the Small Magellanic Cloud", IAU Symp. 291, 459 - 461


• autocitations:
2012:
• Krtička J., Kubát J., 2012, "Influence of extreme ultraviolet radiation on P V ionization fraction in hot star winds", Mon. Not. Roy. Astron. Soc. 427, 84 - 90

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