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Perspectives for observing hot massive stars with XMM-Newton in the years 2017-2027
DOI: 10.1002/asna.201713332
Bibcode: 2017AN....338..207R
Rauw, G.
XMM-Newton has deeply changed our picture of X-ray emission of hot massive stars. High-resolution X-ray spectroscopy, as well as monitoring of these objects, has helped us to gain a deeper insight into the physics of single massive stars with or without magnetic fields, as well as of massive binary systems, where the stellar winds of both stars in…
2017
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Astronomische Nachrichten
XMM-Newton
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