[CII] EMISSION FROM THE MAGELLANIC CLOUDS

被引：1
|
作者：
Israel, F. P. [1 ]
Maloney, P. R. [2 ]
机构：
[1] Leiden Univ, Sterrewacht Leiden, Postbus 9513, NL-2300 RA Leiden, Netherlands
[2] Univ Colorado, CASA, Boulder, CO 80303 USA
来源：
CONDITIONS AND IMPACT OF STAR FORMATION: NEW RESULTS WITH HERSCHEL AND BEYOND | 2011年 / 52卷
关键词：
D O I：
10.1051/eas/1152050
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In the Magellanic Clouds, the [CII]/CO and the [CII]/FIR ratios are much higher than seen in Milky Way star-forming regions. The enhanced relative strength of the [CII] line reflects the physical environment characterised by the low metallicities, dust abundances, and PAH abundances of the LMC, and especially the SMC.
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页码：287 / +
页数：2
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