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...
Main Authors: | , , , |
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Other Authors: | , , |
Format: | Article |
Language: | English |
Published: |
IOP Publishing,
2016-05-18T13:04:12Z.
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Subjects: | |
Online Access: | Get fulltext |