118 citations · 1k across the 30 of their papers we have counts for
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X-ray emission from hydrodynamical simulations in non-LTE wind models
J. Krticka, A. Feldmeier, L. M. Oskinova +2
Hot stars are sources of X-ray emission originating in their winds. Although hydrodynamical simulations that are able to predict this X-ray emission are available, the inclusion of…
Spectroscopy and hydrodynamics of dense stellar winds
W. -R. Hamann, G. Graefener, L. M. Oskinova +1
Analyzing the spectra from Wolf-Rayet stars requires adequate non-LTE modeling of their expanding atmosphere. The numerical schemes for solving the radiative transfer in the co-mov…
Discovery of X-ray Emission from the Wolf-Rayet star WR142 of oxygen subtype
L. M. Oskinova, W. -R. Hamann, A. Feldmeier +2
We report the discovery of weak yet hard X-ray emission from the Wolf-Rayet (WR) star WR142 with the XMM-Newton X-ray telescope. Being of spectral subtype WO2, WR142 is a massive s…