The ISM in NGC 4261

Details The ISM in NGC 4261 The ISM in NGC 4261

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop...78t&link_type=abstract

XMM-Newton Proposal ID #05021201

Mathematics

Logic

Galaxies, Galactic Surveys, Ngc4261, Xmm-Newton Proposal 05021201

Scientific paper

We propose to investigate the spatial and spectral properties of the hot ISM in the nearby early-type galaxy NGC 4261. The galaxy is known to have a very peculiar asymmetric distribution of X-ray sources and of globular clusters, an active nuclear radio source with unique two-sided radio jet and an extended and morphologically disturbed ISM. We will obtain a firm determination of the properties of the fine structure of the hot gas and investigate its relation with both the X-ray binary and globular cluster populations and with the AGN activity.

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