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[CII] emission from the Magellanic Clouds
Published online by Cambridge University Press: 25 November 2011
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.
- Type
- Research Article
- Information
- European Astronomical Society Publications Series , Volume 52: Conditions and Impact of Star Formation , 2011 , pp. 287 - 288
- Copyright
- © EAS, EDP Sciences 2011
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