Characteristics of the ISOCAM mid-infrared emission of early-type galaxies
被引:0
作者:
Madden, SC
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h-index: 0
机构:
CEA Saclay, Serv Astrophys, F-91191 Gif Sur Yvette, FranceCEA Saclay, Serv Astrophys, F-91191 Gif Sur Yvette, France
Madden, SC
[1
]
Vigroux, L
论文数: 0引用数: 0
h-index: 0
机构:
CEA Saclay, Serv Astrophys, F-91191 Gif Sur Yvette, FranceCEA Saclay, Serv Astrophys, F-91191 Gif Sur Yvette, France
Vigroux, L
[1
]
机构:
[1] CEA Saclay, Serv Astrophys, F-91191 Gif Sur Yvette, France
来源:
STAR FORMATION IN EARLY-TYPE GALAXIES
|
1999年
/
163卷
关键词:
D O I:
暂无
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
In order to interprete the mid-infrared emission from early-type galaxies, we have conducted a survey of early-type galaxies using ISOCAM, on board the ISO satellite. With 6 " resolution images of broad bands, centered at 4.5, 6.75 and 15 mu m, we can begin to elucidate the origin and distribution of various components of the mid infrared emission in early-type galaxies.