Resonant Scattering of X-ray Emission Lines in the Hot Intergalactic Medium
- 6 October 2010
- journal article
- Published by Springer Nature in Space Science Reviews
- Vol. 157 (1-4) , 193-209
- https://doi.org/10.1007/s11214-010-9685-4
Abstract
No abstract availableKeywords
All Related Versions
This publication has 37 references indexed in Scilit:
- Resonance scattering, absorption and off-centre abundance peaks in clusters of galaxiesMonthly Notices of the Royal Astronomical Society, 2006
- Determining Distances to Clusters of Galaxies Using Resonant X-Ray Emission LinesThe Astrophysical Journal, 2006
- Spatial Diffusion of X-Ray Emission Lines in the M87 Cooling Flow; Evidence for AbsorptionThe Astrophysical Journal, 2001
- XMM-Newton observations of M 87 and its X-ray haloAstronomy & Astrophysics, 2001
- Iron K-Line mapping of clusters of galaxies with the resonance scattering effectAstronomische Nachrichten, 1999
- How Abundant Is Iron in the Core of the Perseus Cluster?The Astrophysical Journal, 1998
- Resonance Line Scattering Modifies X‐Ray Surface Brightness of Elliptical GalaxiesThe Astrophysical Journal, 1998
- Using X-ray absorption lines to determine the distances to clusters of galaxiesThe Astrophysical Journal, 1989
- Measuring H0 and q0 with X-ray lines from galaxy clustersThe Astrophysical Journal, 1988
- Radiative transfer of X-rays in the solar coronaThe Astrophysical Journal, 1978