XMM-Newton Proposal 02009201

Details XMM-Newton Proposal 02009201 XMM-Newton Proposal 02009201

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop...48b&link_type=abstract

XMM-Newton Proposal ID #02009201

Astronomy and Astrophysics

Astrophysics

M87-Center, Xmm-Newton Proposal 02009201

Scientific paper

The M87 X-ray halo is by far the best place to study several important astrophysical phenomena, like the structure of so-called cooling flows, supernova abundance yields, the interaction of jets with the surrounding intracluster medium (ICM), and how the central galaxy is embedded into the structure of the cluster. The PV phase data have provided already a wide range of spectacular new insights. More precise spectral data are required, however, to draw firm astrophysical conclusions. To this aim we propose a deeper observation of M87.

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