SIMULATING ASTRO-H OBSERVATIONS OF SLOSHING GAS MOTIONS IN THE CORES OF GALAXY CLUSTERS

SIMULATING ASTRO-H OBSERVATIONS OF SLOSHING GAS MOTIONS IN THE CORES OF GALAXY CLUSTERS

Astro-H will be the first X-ray observatory to employ a high-resolution microcalorimeter, capable of measuring the shift and width of individual spectral lines to the precision necessary for estimating the velocity of the diffuse plasma in galaxy clusters. This new capability is expected to bring si...

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Bibliographic Details
Main Authors: Simionescu, A. (Author), Bautz, Marshall W. (Contributor), ZuHone, John A. (Author), Miller, Eric D (Author)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor), ZuHone, J. A. (Contributor), Miller, Eric D. (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2016-05-18T13:04:12Z.
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