The interstellar medium in high-redshift submillimeter galaxies as probed by infrared spectroscopy

Submillimeter galaxies (SMGs) at $z\gtrsim1$ are luminous in the far-infrared and have star-formation rates, SFR, of hundreds to thousands of solar masses per year. However, it is unclear whether they are true analogs of local ULIRGs or whether the mode of their star formation is more similar to tha...

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Bibliographic Details
Main Authors:	Wardlow, J, Cooray, A, Osage, W, Bourne, N, Clements, D, Dannerbauer, H, Dunne, L, Dye, S, Eales, S, Farrah, D, Furlanetto, C, Ibar, E, Ivison, R, Maddox, S, Michałowski, M, Riechers, D, Rigopoulou, D, Scott, D, Smith, M, Wang, L, Werf, P, Valiante, E, Valtchanov, I, Verma, A
Format:	Journal article
Published:	IOP Publishing 2017

The interstellar medium in high-redshift submillimeter galaxies as probed by infrared spectroscopy

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