A new paradigm for the X-ray emission of O stars from XMM-Newton observations of the O9.7 supergiant $\zeta$ Orionis

Publisher： Edp Sciences

E-ISSN： 1432-0746|463|3|1111-1123

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.463, Iss.3, 2007-03, pp. : 1111-1123

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