X-raying cosmic star formation history

被引:0
|
作者
Wang, YP
Yamada, T
Taniguchi, Y
机构
关键词
D O I
10.1017/S1743921304003205
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Based on our previous work about a co-evolution of massive black holes (MBH) and their host spheroids, we estimate the cosmic star formation history associated with AGN accretion by ROSAT X-ray All sky surveys. We show: 1) the total amount of star formation associated with MBH growth is at least half of the net star formation at high redshift, which probably totally missed by the current UV/optical deep surveys; 2) the FIR emission from the dust heated by star formation on-going during the MBH growth could be a significant energy source for SCUBA populations; 3)the peak redshift of the massive spheroid formation in this case is around 1.5, not necessary to be at much higher redshift.
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页码:541 / 542
页数:2
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