Astronomy and Astrophysics – Astronomy
Scientific paper
May 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aspc..289..267w&link_type=abstract
The Proceedings of the IAU 8th Asian-Pacific Regional Meeting, Volume I, held 2-5 July 2002 at National Center of Sciences, Hito
Astronomy and Astrophysics
Astronomy
Scientific paper
Based on our previous work about a joint evolution and the consequential black hole to bulge mass correlation, we use the observed X-ray luminosity function of AGNs and their evolution to estimate the star formation history which is associated with the black hole growth. We show that the total amount of star formation associated with the massive black hole growth is almost the same as that detected by the current optical deep surveys. Meanwhile, the far infrared emission from the dust heated by star formation on-going during the black hole growth could sufficiently account for the observed SCUBA counts, and would be the good candidates of the SCUBA population.
Taniguchi Yoshiaki
Wang Ya-Ping
Yamada Toru
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