Determining the Distance of Cyg X-3 with its X-Ray Dust Scattering Halo

Using a cross-correlation method, we study the X-ray halo of Cyg X-3. Two components of dust distributions are needed to explain the time lags derived by the cross-correlation method. Assuming the distance as 1.7 kpc for Cyg OB2 association (a richest OB association in the local Galaxy) and another...

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Bibliographic Details
Published inThe Astrophysical journal Vol. 695; no. 2; pp. 1111 - 1120
Main Authors Ling, Zhixing, Zhang, Shuang Nan, Tang, Shichao
Format Journal Article
LanguageEnglish
Published Bristol IOP Publishing 20.04.2009
IOP
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