2011A&A...526A..32M

Muijres, L. E.; de Koter, A.; Vink, J. S.; Krtička, J.; Kubát, J.; Langer, N. 2011, "Predictions of the effect of clumping on the mass-loss rates of O-type stars", Astron. Astrophys. 526, A32

• pdf, a copy for personal use: *
• some citations:
2011:
1. Ortiz-León, G. N.; Loinard, L.; Rodríguez, L. F.; Mioduszewski, A. J.; Dzib, S. A.; 2011, "Mass loss from inhomogeneous hot star winds. I. Resonance line formation in 2D models", Astrophys. J. 737, 30

2012:
2. Ekström, S.; Georgy, C.; Eggenberger, P.; Meynet, G.; Mowlavi, N.; Wyttenbach, A.; Granada, A.; Decressin, T.; Hirschi, R.; Frischknecht, U.; Charbonnel, C.; Maeder, A. 2012, "Grids of stellar models with rotation. I. Models from 0.8 to 120 M_sun at solar metallicity (Z = 0.014)", Astron. Astrophys. 537, A146
3. Ignace, R.; Waldron, W. L.; Cassinelli, J. P., Burke, A. E., 2012, "X-ray Emission Line Profiles from Wind Clump Bow Shocks in Massive Stars", Astrophys. J.750, 40
4. Prinja, R. K.; Massa, D. L.; Urbaneja, M. A.; Kudritzki, R.-P., 2012, "PN fast winds: temporal structure and stellar rotation", Mon. Not. Roy. Astron. Soc. 422, 3142 - 3150
5. Georgy, C.; Ekström, S.; Meynet, G.; Massey, P.; Levesque, E. M.; Hirschi, R.; Eggenberger, P.; Maeder, A., 2012, "Grids of stellar models with rotation II. WR populations and supernovae/GRB progenitors at Z = 0.014", Astron. Astrophys. 542, A29
6. 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
7. Sundqvist J. O., Owocki S. P., 2012, "Diagnosing small- and large-scale structure in the winds of hot, massive OB-stars", in Circumstellar Dynamics at High Resolution, A. C. Carciofi & T. Rivinius eds., ASP Conf. Ser. Vol. 464, p. 301
8. Sundqvist J. O., Owocki S. P., 2012, "Clumping in the inner winds of hot, massive stars from hydrodynamical line-driven instability simulations", Mon. Not. Roy. Astron. Soc. 428, 1837 - 1844

2013:
9. 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
10. Dzib S. A., Rodriguez L. F., Loinard L., Mioduszewski A. J., Ortiz-Leon G. N., Araudo A. T., 2012, "Multi-Epoch VLBA Observations of the Compact Wind-Collision Region in the Quadruple System Cyg OB2 #5", Astrophys. J. 763, 139
11. Yusof N., Hirschi R., Meynet G., Crowther P. A., Ekström S., Frischknecht U., Georgy C., Abu Kassim H., Schnurr O., 2013. "Evolution and fate of very massive stars", Mon. Not. Roy. Astron. Soc. 433, 1114 - 1132

2014:
12. 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
13. 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
14. 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:
15. Hirschi, R., 2015, "Mass-Loss Rates of Very Massive Stars", in Very Massive Stars in the Local Universe, Astrophysics and Space Science Library, Volume 412, Springer, p. 157
16. Puls, J.; Sundqvist, J. O.; Markova, N., 2015, "Physics of Mass Loss in Massive Stars", in New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry, IAU Symp. 307, p. 25 - 36
17. Bouret, J.-C.; Lanz, T.; Hillier, D. J.; Martins, F.; Marcolino, W. L. F.; Depagne, E., 2015, "No breakdown of the radiatively driven wind theory in low-metallicity environments", Mon. Not. Roy. Astron. Soc. 449, 1545 - 1569


• weak autocitations:
2011:
1. Vink, J. S.; Muijres, L. E.; Anthonisse, B.; de Koter, A.; Gräfener, G.; Langer, N.; 2011, "Wind modelling of very massive stars up to 300 solar masses", Astron. Astrophys. 531, A132

2012:
2. Muijres, L. E.; Vink, Jorick S.; de Koter, A.; Müller, P. E.; Langer, N.; 2012, "Predictions for mass-loss rates and terminal wind velocities of massive O-type stars", Astron. Astrophys. 537, A37
3. Vink, Jorick S.; Gräfener, Götz; 2012, "The Transition Mass-loss Rate: Calibrating the Role of Line-driven Winds in Massive Star Evolution", Astrophys. J. 751, L34
4. Vink J. S., 2012, "Linear spectropolarimetry and the circumstellar media of young and massive stars", in Stellar polarimetry: form birth to death, AIP Conf. Proc. Vol. 1429, pp. 147 - 158
5. Langer N., 2012, "Presupernova Evolution of Massive Single and Binary Stars", Ann. Rev. Astron. Astrophys. 50, 107 - 164
6. Gvaramadze, V. V.; Langer, N.; Mackey, J., 2012, "ζ Oph and the weak-wind problem", Mon. Not. Roy. Astron. Soc. 427, L50 - L54

2015:
7. Vink, J. S., 2015, "Mass-Loss Rates of Very Massive Stars", in Very Massive Stars in the Local Universe, Astrophysics and Space Science Library, Volume 412, Springer, p. 77
8. Sanyal, D.; Grassitelli, L.; Langer, N.; Bestenlehner, J. M., 2015, "Massive main-sequence stars evolving at the Eddington limit", Astron. Astrophys. 580, A20
9. Shenar, T.; Oskinova, L.; Hamann, W.-R.; Corcoran, M. F.; Moffat, A. F. J.; Pablo, H.; Richardson, N. D.; Waldron, W. L.; Huenemoerder, D. P.; Maíz Apellániz, J.; Nichols, J. S.; Todt, H.; Nazé, Y.; Hoffman, J. L.; Pollock, A. M. T.; Negueruela, I., 2015, "A Coordinated X-Ray and Optical Campaign of the Nearest Massive Eclipsing Binary, δ Orionis Aa. IV. A Multiwavelength, Non-LTE Spectroscopic Analysis", Astrophys. J. 809, 135


• autocitations:
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., 2012, "Influence of extreme ultraviolet radiation on P V ionization fraction in hot star winds", Mon. Not. Roy. Astron. Soc. 427, 84 - 90
• Kubát J., Šurlan B., 2012, "Validity of clumping approximations for mass-loss rates determination", in Four Decades of Research on Massive Stars, C. Robert, N. St-Louis & L. Drissen eds., Astron. Soc. Pacific. Conf. Ser. Vol. 465, p. 128
2014:
• Šurlan B., Hamann W.-R., Aret A., Kubát J., Oskinova L. M., Torres A. F., 2013, "Macroclumping as solution of the discrepancy between Hα and P v mass loss diagnostics for O-type stars", Astron. Astrophys. 559, A130

---