[C II] emission in z ~ 6 strongly lensed, star-forming galaxies
The far-infrared fine-structure line [C ii] at 1900.5 GHz is known to be one of the brightest cooling lines in local galaxies, and therefore it has been suggested to be an efficient tracer for star formation in very high redshift galaxies. However, recent results for galaxies at z > 6 have yielde...
| Main Authors: | , , , , , , , |
|---|---|
| Format: | Journal Article |
| Published: |
Oxford
2016
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| Online Access: | http://hdl.handle.net/20.500.11937/23388 |
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