Determining interstellar dust properties with scattered X-ray halo
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Geology
Link
http://link.springer.com/content/pdf/10.5047/eps.2011.02.004
Reference17 articles.
1. Hu, J. et al., A new method to determine the distances of variable galactic X-ray sources, Astrophys. J., 614, L45–L48, 2004.
2. Lee, J. C. and B. Ravel, Determining the grain composition of the interstellar medium with high-resolution X-ray spectroscopy, Astrophys. J., 622, 970–976, 2005.
3. Lee, J. C. et al., Condensed matter astrophysics: a prescription for determining the species-specific composition and quantity of interstellar dust using X-rays, Astrophys. J., 702, 970–979, 2009.
4. Ling, Z. et al., A study of the X-ray dust scattering halo of Cyg X-1 with a cross-correlation method, Astrophys. J., 690, 224–230, 2009a.
5. Ling, Z. et al., Determining the distance of Cyg X-3 with its X-ray dust scattering halo, Astrophys. J., 695, 1111–1120, 2009b.
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