Mid-IR Radiation of 3C Radio Galaxies II. Results

Details Mid-IR Radiation of 3C Radio Galaxies II. Results Mid-IR Radiation of 3C Radio Galaxies II. Results

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.511..271f&link_type=abstract

Exploiting the ISO Data Archive. Infrared Astronomy in the Internet Age, held in Siguenza, Spain 24-27 June, 2002. Edited by

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The spectral energy distribution of 3C galaxies was constructed by compiling measurements in optical, near IR, far-IR and at mm bands for galaxies detected in our ISOCAM survey. Exploiting the models discussed by Siebenmorgen et al. (2002, hereafter SFK), we argue that for a large fraction of the detected galaxies, hot dust is the most likely explanation for the mid-infrared emission. Where this is the case, we have derived the total infrared luminosities, dust mass and limits on the dust temperatures. Taking into account selection biases in our sample, we discuss the frequency and properties of hot dust in radio galaxies at high redshift.

Affiliated with

Also associated with

No associations

Rating

Mid-IR Radiation of 3C Radio Galaxies II. Results does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Mid-IR Radiation of 3C Radio Galaxies II. Results, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mid-IR Radiation of 3C Radio Galaxies II. Results will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-921075