Computer Science
Scientific paper
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.
Feruglio Chiara
Fiore Fabrizio
Lanzuisi Giorgio
Maiolino Roberto
Piconcelli Enrico
No associations
LandOfFree
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.
Profile ID: LFWR-SCP-O-1110171