EVN and MERLIN observations of a complete sample of ultra luminous infrared galaxies

被引：0
|
作者：
Polatidis, AG [1 ]
Conway, JE [1 ]
Pihlström, Y [1 ]
机构：
[1] Max Planck Inst Radioastron, D-5300 Bonn, Germany
来源：
NEUTRAL ISM IN STARBURST GALAXIES | 2004年 / 320卷
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D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Radio imaging of ULIR galaxies is ideal to explore the connection between the starburst and the AGN phenomenon since it is unaffected by dust obscuration, and provides the required high angular resolution to distinguish between an AGN and starburst emission at the centres of these galaxies. We present lambda 18cm radio continuum, EVN and MERLIN observations of two ULIRGs (from a sample of 13), and assess the contribution of an AGN or a starburst to the total energy distribution.
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页码：226 / 229
页数：4
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