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Cited article:
L. Koesterke , W.-R. Hamann , G. Gräfener
A&A, 384 2 (2002) 562-567
Published online: 2002-03-15
This article has been cited by the following article(s):
23 articles
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Three-dimensional modeling of chromospheric spectral lines in a simulated active region
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A massive white-dwarf merger product before final collapse
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Coupling hydrodynamics with comoving frame radiative transfer
A. A. C. Sander, W.-R. Hamann, H. Todt, R. Hainich and T. Shenar Astronomy & Astrophysics 603 A86 (2017) https://doi.org/10.1051/0004-6361/201730642
Recent advances in non-LTE stellar atmosphere models
Andreas A. C. Sander Proceedings of the International Astronomical Union 12 (S329) 215 (2016) https://doi.org/10.1017/S1743921317003362
Light-travel-time diagnostics in early supernova spectra: substantial mass-loss of the IIb progenitor of SN 2013cu through a superwind
G. Gräfener and J. S. Vink Monthly Notices of the Royal Astronomical Society 455 (1) 112 (2016) https://doi.org/10.1093/mnras/stv2283
The VLT-FLAMES Tarantula Survey
J. M. Bestenlehner, G. Gräfener, J. S. Vink, et al. Astronomy & Astrophysics 570 A38 (2014) https://doi.org/10.1051/0004-6361/201423643
Planets, Stars and Stellar Systems
Ivan Hubeny Planets, Stars and Stellar Systems 51 (2013) https://doi.org/10.1007/978-94-007-5615-1_2
Stellar mass-loss near the Eddington limit
G. Gräfener and J. S. Vink Astronomy & Astrophysics 560 A6 (2013) https://doi.org/10.1051/0004-6361/201321914
THE ABUNDANCES OF NEUTRON-CAPTURE SPECIES IN THE VERY METAL-POOR GLOBULAR CLUSTER M15: A UNIFORM ANALYSIS OF RED GIANT BRANCH AND RED HORIZONTAL BRANCH STARS
Jennifer S. Sobeck, Robert P. Kraft, Christopher Sneden, et al. The Astronomical Journal 141 (6) 175 (2011) https://doi.org/10.1088/0004-6256/141/6/175
Basic Tools for Modeling Stellar and Planetary Atmospheres
Ivan Hubeny Proceedings of the International Astronomical Union 7 (S282) 221 (2011) https://doi.org/10.1017/S1743921311027414
Ivan Hubeny and Thierry Lanz 1 (2009) https://doi.org/10.1007/978-0-387-87621-4_30
Mass loss from late-type WN stars and itsZ-dependence
G. Gräfener and W.-R. Hamann Astronomy & Astrophysics 482 (3) 945 (2008) https://doi.org/10.1051/0004-6361:20066176
Modeling Ultraviolet Wind Line Variability in Massive Hot Stars
A. Lobel and R. Blomme The Astrophysical Journal 678 (1) 408 (2008) https://doi.org/10.1086/529129
Wolf-Rayet Wind Models from Hydrodynamic Model Atmospheres
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Lower mass loss rates in O-type stars: Spectral signatures of dense clumps
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Hydrodynamic model atmospheres for WR stars
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Comprehensive modelling of the planetary nebula LMC-SMP 61 and its [WC]-type central star
G. Stasińska, G. Gräfener, M. Peña, et al. Astronomy & Astrophysics 413 (1) 329 (2004) https://doi.org/10.1051/0004-6361:20034072
Grids of model spectra for WN stars, ready for use
W.-R. Hamann and G. Gräfener Astronomy & Astrophysics 427 (2) 697 (2004) https://doi.org/10.1051/0004-6361:20040506
A Grid of Non‐LTE Line‐blanketed Model Atmospheres of O‐Type Stars
Thierry Lanz and Ivan Hubeny The Astrophysical Journal Supplement Series 146 (2) 417 (2003) https://doi.org/10.1086/374373
Quantitative Spectroscopy of O Stars at Low Metallicity: O Dwarfs in NGC 346
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Hydrodynamic model atmospheres for hot stars
Götz Gräfener and Wolf-Rainer Hamann Symposium - International Astronomical Union 212 190 (2003) https://doi.org/10.1017/S0074180900211960
Line-blanketed model atmospheres for WR stars
G. Gräfener, L. Koesterke and W.-R. Hamann Astronomy & Astrophysics 387 (1) 244 (2002) https://doi.org/10.1051/0004-6361:20020269