The nature of ISOCAM galaxies in the Hubble Deep Field South

被引:0
|
作者
Rigopoulou, D [1 ]
Franceschini, A [1 ]
Genzel, R [1 ]
机构
[1] Max Planck Inst Extraterr Phys, D-85741 Garching, Germany
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P1 [天文学];
学科分类号
0704 ;
摘要
The various deep ISOCAM surveys revealed a new class of infrared luminous galaxies which are characterized by a high rate of evolution and are found at redshifts of zsimilar to1. Here we report results of our near-infrared VLT-ISAAC spectroscopic survey aimed at characterising the nature of these sources. We find that the rest-frame R-band spectra resemble those of powerful dust enshrouded starbursts. More recent detailed studies revealed that some of these systems are in fact extremely massive galaxies.
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页码:255 / 260
页数:6
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