Publisher： Edp Sciences
E-ISSN： 1638-1963|52|issue|287-288
ISSN： 1633-4760
Source： EAS Publications Series, Vol.52, Iss.issue, 2011-11, pp. : 287-288
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Abstract
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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