A Study of the X-Ray Dust Scattering Halo of Cyg X-1 with a Cross-Correlation Method
X-ray photons scattered by the interstellar medium carry information about dust distribution, dust grain model, scattering cross section, and the distance of the source; they also take a longer time than unscattered photons to reach the observer. Using a cross-correlation method, we study the light...
Saved in:
Published in | The Astrophysical journal Vol. 690; no. 1; pp. 224 - 230 |
---|---|
Main Authors | , , , |
Format | Journal Article |
Language | English |
Published |
Bristol
IOP Publishing
01.01.2009
IOP |
Subjects | |
Online Access | Get full text |
Cover
Loading…
Be the first to leave a comment!