The IR to X-rays SED of the Heavily Obscured Quasar IRAS 09104+4109

Details The IR to X-rays SED of the Heavily Obscured Quasar IRAS 09104+4109 The IR to X-rays SED of the Heavily Obscured Quasar IRAS 09104+4109

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1126..242l&link_type=abstract

SIMBOL-X: FOCUSING ON THE HARD X-RAY UNIVERSE: Proceedings of the 2nd International Simbol-X Symposium. AIP Conference Proceedi

Computer Science

Active And Peculiar Galaxies And Related Systems, Galactic Nuclei, Circumnuclear Matter, And Bulges, Quasars, Photometric, Polarimetric, And Spectroscopic Instrumentation, Spectroscopy And Spectrophotometry

Scientific paper

Constraining the NH distribution of AGNs at high column densities and high X-ray luminosites is crucial to provide a reliable MIR/X-ray luminosity ratio distribution and compare it with the expectations of dust reprocessing models. Here we present the IR to X-rays broad band SED of of the hyperluminous infrared galaxy and Type 2 quasar IRAS 09104+4109 (z = 0.442), taking into account our recent result suggesting the likely Compton-thin nature of its absorber.

Affiliated with

Also associated with

No associations

Rating

The IR to X-rays SED of the Heavily Obscured Quasar IRAS 09104+4109 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 The IR to X-rays SED of the Heavily Obscured Quasar IRAS 09104+4109, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The IR to X-rays SED of the Heavily Obscured Quasar IRAS 09104+4109 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1110171