[CII] emission from the Magellanic Clouds

Details [CII] emission from the Magellanic Clouds [CII] emission from the Magellanic Clouds

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011eas....52..287i&link_type=abstract

EAS Publications Series, Volume 52, 2011, pp.287-288

Physics

Scientific paper

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.

Affiliated with

Also associated with

No associations

Rating

[CII] emission from the Magellanic Clouds does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with [CII] emission from the Magellanic Clouds, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and [CII] emission from the Magellanic Clouds will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-737664