What drives the [CII]/FIR deficit in submillimeter galaxies?
2019 ◽
Vol 15
(S352)
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pp. 293-294
AbstractSubmillimeter galaxies at redshift z⩾1 show a pronounced [CII]/FIR deficit down to sub-kpc scales; however, the physical origin of this deficit remains poorly understood. We use resolved ALMA observations of the [CII], FIR and CO(3–2) emission in two z = 3 SMGs to distinguish between the different proposed scenarios; the thermal saturation of the [CII] emission is the most likely explanation.
1997 ◽
Vol 161
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pp. 505-510
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2013 ◽
Vol 438
(1)
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pp. 657-662
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2011 ◽
Vol 115
(29)
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pp. 14111-14122
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