Computer Science
Scientific paper
Sep 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006cxo..prop.2209f&link_type=abstract
Chandra Proposal ID #08700576
Computer Science
Chandra Proposal Id #08700576
Scientific paper
We propose to study the interactions of AGN outbursts with their environments through an observation of two radio sources, PKS0123-016A and 3C40, associated with NGC541 and NGC547. Both galaxies lie in the cluster A194 and are surrounded by small X-ray coronae. Using a VLA observation, we will compare the coronal gas parameters (density, temperature, pressure) with the radio structure to understand how powerful AGN channel energy through tenuous coronae. We will measure the source spectrum, detect individual luminous X-ray sources, and compare the radio and X-ray structure of Minkowski's object, a local example of jet-induced star formation that lies along the jet emanating from NGC541. We will search for jet emission from both 3C40 and PKS0123-016A and study the hotspot in PKS0123-016A.
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