204 citations · 5k across the 190 of their papers we have counts for
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A detailed X-ray investigation of zeta Puppis - The variability on short and long timescales
Yael Naze, Lidia M. Oskinova, Eric Gosset
Stellar winds are a crucial component of massive stars, but their exact properties still remain uncertain. To shed some light on this subject, we have analyzed an exceptional set o…
A Report on the X-ray Properties of the tau Sco Like Stars
Richard Ignace, Lidia Oskinova, Derck Mass
An increasing number of OB stars have been shown to possess magnetic fields. Although the sample remains small, it is surprising that the magnetic and X-ray properties of these sta…
Clumped stellar winds in supergiant high-mass X-ray binaries
L. M. Oskinova, A. Feldmeier, P. Kretschmar
The clumping of massive star winds is an established paradigm, which is confirmed by multiple lines of evidence and is supported by stellar wind theory. We use the results from tim…
The slow X-ray pulsar SXP 1062 and associated supernova remnant in the Wing of the Small Magellanic Cloud
L. M. Oskinova, M. A. Guerrero, V. Henault-Brunet +6
SXP 1062 is an exceptional case of a young neutron star in a wind-fed high-mass X-ray binary associated with a supernova remnant. A unique combination of measured spin period, its…
On the Weak-Wind Problem in Massive Stars: X-ray Spectra Reveal a Massive Hot Wind in μ Columbae
David P. Huenemoerder, Lidia M. Oskinova, Richard Ignace +4
μ Columbae is a prototypical weak-wind O-star for which we have obtained a high-resolution X-ray spectrum with the Chandra LETG/ACIS-S instrument and a low resolution spectrum with…
A rare early-type star revealed in the Wing of the Small Magellanic Cloud
C. J. Evans, R. Hainich, L. M. Oskinova +6
Sk 183 is the visually-brightest star in the N90 nebula, a young star-forming region in the Wing of the Small Magellanic Cloud (SMC). We present new optical spectroscopy from the V…