Do sub-mm sources and quasars form an evolutionary sequence?

被引:4
作者
Almaini, O [1 ]
机构
[1] Royal Observ, Astron Inst, Edinburgh EH9 3HJ, Midlothian, Scotland
关键词
quasars : general; galaxies : formation; galaxies : evolution; gravitational lensing; X-rays;
D O I
10.1002/asna.200310028
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The high redshift sub-mm sources discovered by SCUBA are widely believed to represent the dust-enshrouded formation of massive elliptical galaxies. Given the strong evidence for a link between the formation of the spheroid and the growth of the central black hole, one might expect to see a luminous quasar at the nucleus of every SCUBA source. Somewhat surprisingly, however, only a very small fraction (similar to 5%) are detected in X-rays, In this paper I discuss some of the implications of these results and discuss the accumulating evidence that sub-mm sources and quasars may represent different stages in the evolutionary sequence of a massive proto-spheroid.
引用
收藏
页码:109 / 112
页数:4
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