L. M. Oskinova

A COORDINATED X-RAY AND OPTICAL CAMPAIGN OF THE NEAREST MASSIVE ECLIPSING BINARY,<i>δ</i>ORIONIS Aa. IV. A MULTIWAVELENGTH, NON-LTE SPECTROSCOPIC ANALYSIS

T. Shenar, L. M. Oskinova, W.‐R. Hamann et al. · The Astrophysical Journal · 2015 · 279 citations · Full text

Natural Sciences, Astronomy, Physics +17

The Wolf-Rayet stars in the Large Magellanic Cloud

R. Hainich, U. Rühling, H. Todt et al. · Astronomy and Astrophysics · 2014 · 199 citations · Full text

Natural Sciences, Astronomy, Physics +17

Neglecting the porosity of hot-star winds can lead to underestimating mass-loss rates

L. M. Oskinova, W.‐R. Hamann, A. Feldmeier · Springer Link (Chiba Institute of Technology) · 2007 · 149 citations · Full text

Natural Sciences, Astronomy, Physics +16

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 et al. · Space Science Reviews · 2017 · 141 citations · Full text

Natural Sciences, Astronomy, Physics +15

Clumping in hot-star winds

W.‐R. Hamann, Achim Feldmeier, L. M. Oskinova · 2008 · 134 citations

Natural Sciences, Astronomy, Physics +9