The dominant heating mechanism for the dust in powerful AGN

Details The dominant heating mechanism for the dust in powerful AGN The dominant heating mechanism for the dust in powerful AGN

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atnf.prop..129m&link_type=abstract

ATNF proposal C1537, Semester: April, 2006

Computer Science

Extragalactic, Atca

Scientific paper

We are engaged in a major survey of southern 2Jy radio sources with the Spitzer Space Telescope that is aimed at determining the dominant heating mechanism from the mid- to far-IR (MFIR) emitting dust in radio-loud AGN. An important part of this work is to determine the degree of contamination of the far-IR continuum by synchrotron-emitting components in the Spitzer beam. Therefore we propose to make 22GHz radio observations of all of the objects with delta < -25 degrees in our sample with ATCA, in order to determine the high frequency spectral indices of the core radio components.

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