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Some Developments of the Weak Stellar Magnetic Field Determination Method for the Example of Cygnus X-1
Published online by Cambridge University Press: 23 April 2012
Abstract
Some developments of measurements of the weak stellar magnetic fields by the least square technique applied to spectropolarimetric data are proposed and used for the X-ray binary Cyg X-1 = HDE 226868 (the optical counterpart is an O 9.7 supergiant).
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- Copyright © International Astronomical Union 2012