| Neglecting the porosity of hot-star winds can lead to underestimating mass-loss rates LM Oskinova, WR Hamann, A Feldmeier Astronomy & Astrophysics 476 (3), 1331-1340, 2007 | 270 | 2007 |
| The Wolf-Rayet stars in the Large Magellanic Cloud-A comprehensive analysis of the WN class R Hainich, U Rühling, H Todt, LM Oskinova, A Liermann, G Gräfener, ... Astronomy & Astrophysics 565, A27, 2014 | 197 | 2014 |
| High-resolution X-ray spectroscopy of bright O-type stars LM Oskinova, A Feldmeier, WR Hamann Monthly Notices of the Royal Astronomical Society 372 (1), 313-326, 2006 | 155 | 2006 |
| Evolution of X-ray emission from young massive star clusters LM Oskinova Monthly Notices of the Royal Astronomical Society 361 (2), 679-694, 2005 | 146 | 2005 |
| An introduction to the chandra carina complex project LK Townsley, PS Broos, MF Corcoran, ED Feigelson, M Gagné, ... The Astrophysical Journal Supplement Series 194 (1), 1, 2011 | 130 | 2011 |
| X-ray line emission from a fragmented stellar wind A Feldmeier, L Oskinova, WR Hamann Astronomy & Astrophysics 403 (1), 217-224, 2003 | 125 | 2003 |
| Macroclumping as solution of the discrepancy between Hα and P v mass loss diagnostics for O-type stars B Šurlan, WR Hamann, A Aret, J Kubat, LM Oskinova, AF Torres Astronomy & Astrophysics 559, A130, 2013 | 123 | 2013 |
| Global X-ray properties of the O and B stars in Carina Y Nazé, PS Broos, L Oskinova, LK Townsley, D Cohen, MF Corcoran, ... The Astrophysical Journal Supplement Series 194 (1), 7, 2011 | 121 | 2011 |
| Towards a unified view of inhomogeneous stellar winds in isolated supergiant stars and supergiant high mass X-ray binaries S Martínez-Núñez, P Kretschmar, E Bozzo, LM Oskinova, J Puls, L Sidoli, ... Space Science Reviews 212, 59-150, 2017 | 120 | 2017 |
| Early magnetic B-type stars: X-ray emission and wind properties LM Oskinova, H Todt, R Ignace, JC Brown, JP Cassinelli, WR Hamann Monthly Notices of the Royal Astronomical Society 416 (2), 1456-1474, 2011 | 117 | 2011 |
| Clumped stellar winds in supergiant high‐mass X‐ray binaries: X‐ray variability and photoionization LM Oskinova, A Feldmeier, P Kretschmar Monthly Notices of the Royal Astronomical Society 421 (4), 2820-2831, 2012 | 114 | 2012 |
| Wolf-Rayet stars in the Small Magellanic Cloud-II. Analysis of the binaries T Shenar, R Hainich, H Todt, A Sander, WR Hamann, AFJ Moffat, ... Astronomy & Astrophysics 591, A22, 2016 | 100 | 2016 |
| The galactic WN stars revisited-Impact of Gaia distances on fundamental stellar parameters WR Hamann, G Gräfener, A Liermann, R Hainich, AAC Sander, T Shenar, ... Astronomy & Astrophysics 625, A57, 2019 | 98 | 2019 |
| Three-dimensional radiative transfer in clumped hot star winds-I. Influence of clumping on the resonance line formation B Šurlan, WR Hamann, J Kubát, LM Oskinova, A Feldmeier Astronomy & Astrophysics 541, A37, 2012 | 95 | 2012 |
| The Galactic WC and WO stars-The impact of revised distances from Gaia DR2 and their role as massive black hole progenitors AAC Sander, WR Hamann, H Todt, R Hainich, T Shenar, ... Astronomy & Astrophysics 621, A92, 2019 | 93 | 2019 |
| Testing massive star evolution, star formation history, and feedback at low metallicity-Spectroscopic analysis of OB stars in the SMC Wing V Ramachandran, WR Hamann, LM Oskinova, JS Gallagher, R Hainich, ... Astronomy & Astrophysics 625, A104, 2019 | 90 | 2019 |
| Carina OB Stars: X-ray Signatures of Wind Shocks and Magnetic Fields M Gagné, G Fehon, MR Savoy, DH Cohen, LK Townsley, PS Broos, ... The Astrophysical Journal Supplement Series 194 (1), 5, 2011 | 90 | 2011 |
| X-ray emission lines from inhomogeneous stellar winds LM Oskinova, A Feldmeier, WR Hamann Astronomy & Astrophysics 422 (2), 675-691, 2004 | 90 | 2004 |
| The conspicuous absence of X-ray emission from carbon-enriched Wolf-Rayet stars LM Oskinova, R Ignace, WR Hamann, AMT Pollock, JC Brown Astronomy & Astrophysics 402 (2), 755-765, 2003 | 89 | 2003 |
| The Quintuplet cluster-I. A K-band spectral catalog of stellar sources A Liermann, WR Hamann, LM Oskinova Astronomy & Astrophysics 494 (3), 1137-1166, 2009 | 84 | 2009 |
