Spectral-Spatial Diagnostics of the Most Luminous X-Ray Cluster of Galaxies with the HETG

Details Spectral-Spatial Diagnostics of the Most Luminous X-Ray Cluster of Galaxies with the HETG Spectral-Spatial Diagnostics of the Most Luminous X-Ray Cluster of Galaxies with the HETG

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cxo..prop..697k&link_type=abstract

Chandra Proposal ID #02800732

Computer Science

Chandra Proposal Id #02800732

Scientific paper

We propose a 100 ks observation of RXJ 1347.5-1145, the most luminous X-ray cluster of galaxies with the HETG. RXJ 1347.5-1145 is a compact high redshift (0.451) X-ray cluster. By using the dispersed spectrum of the HETG and the spatially resolved zero-order image, we plan to measure its cooling flow and detect a number of emission lines of RXJ 1347.5-1145. The observed spectral-spatial properties will determine the dynamics of X-ray gas early in the history of cluster formation.

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