Testing the companion hypothesis for the origin of the X-ray emission from intermediate-mass main-sequence stars

Publisher: Edp Sciences

E-ISSN: 1432-0746|452|3|1001-1010

ISSN: 0004-6361

Source: Astronomy & Astrophysics, Vol.452, Iss.3, 2006-06, pp. : 1001-1010

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