| PROPOSAL OVERVIEW | |
| Proposal Title | Velocity dispersion of the ICM in 3 Disturbed X-ray luminous cool core clusters |
| Proposal Category | Galaxies, Groups of Galaxies, Clusters of Galaxies and Superclusters |
| Proposal Type | LARGE PROGRAM |
| Proposal Id | 084058 |
| Number of Observations | 6 |
| Total exposure time (ks) | 720 |
| PI DETAILS | |
| PI | Prof Andrew Fabian |
| Institute | Institute of Astronomy |
| Country | UNITED KINGDOM |
| CO-INVESTIGATORS | ||
| Name | Country | |
| C. Pinto | UNITED KINGDOM | |
| H. Russell | UNITED KINGDOM | |
| J. Sanders | GERMANY | |
| H. Liu | UNITED KINGDOM | |
| B. McNamara | CANADA | |
| ABSTRACT | |
| We propose to observe 3 X-ray luminous clusters which each have over 10^10 Msun of cold molecular gas in their X-ray cool cores. The ALMA velocity and morphology data indicate that the cold gas is disturbed in these object. If, as Hitomi has shown in the Perseus cluster, the cold gas and ICM share the same velocity field, then we shall measure velocity broadening of the soft X-ray emission lines with the XMM RGS. We shall also measure or constrain mass cooling rates of the ICM below 1-2 keV. | |
| PAPERS |
| - CLASS 1: | papers that present specific XMM-Newton observations |
| - CLASS 2: | papers that refer to published XMM-Newton results with complementary observations, follow-up analysis, or theoretical analysis |
| - CLASS 3: | further deliveries which resulted from the program and which are made available to the community (e.g. source catalogues, processed images or spectra in public data base) |
| - CLASS 4: | comments and suggestions from PI |
| CLASS 1 (1 references) |
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