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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Published in | The Astrophysical journal Vol. 695; no. 2; pp. 1111 - 1120 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
Published |
Bristol
IOP Publishing
20.04.2009
IOP |
Subjects | |
Online Access | Get full text |
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