Computer Science
Scientific paper
Oct 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop...54e&link_type=abstract
XMM-Newton Proposal ID #05016502
Computer Science
Galaxies, Galactic Surveys, Ngc 1097, Ngc 7552, Xmm-Newton Proposal 05016502
Scientific paper
We propose XMM-Newton observations of three barred galaxies selected for their strong radio emission and remarkable magnetic field structures. EPIC spatial and spectral information will be used in combination with our radio data to study the influence of bar lengths and compression strengths on the enhancement of circumnuclear star formation and nuclear activity. We will study the effects of magnetic fields on the evolution of diffuse X-ray halos generated by hot gas outflowing from starforming regions. We will investigate if the distribution of point-like sources, especially ULXs, is correlated with starforming regions at the ends of the bars. EPIC data will be complemented with Chandra observations to disentangle nuclear and circumnuclear emission.
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