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

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

Submillimeter galaxies (SMGs) at 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 that in local...

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Bibliographic Details
Main Authors: Wardlow, J.L., Cooray, A., Osage, Willow, Bourne, Nathan, Clements, David, Dannerbauer, Helmut, Dunne, Loretta, Dye, S., Eales, S., Farrah, Duncan, Furlanetto, C., Ibar, E., Ivison, Rob J., Maddox, S., Michałowski, Michał M., Riechers, Dominik, Rigopoulou, D., Scott, Douglas, Smith, M.W.L., Wang, Lingyu, van der Werf, Paul, Valiante, Elisabetta, Valtchanov, I., Verma, Aprajita
Format: Article
Published: American Astronomical Society 2017
Subjects:
Galaxies: high-redshift
Galaxies: ISM
Galaxies: star formation
Gravitational lensing: strong submillimeter
Online Access:https://eprints.nottingham.ac.uk/42340/

Internet

https://eprints.nottingham.ac.uk/42340/

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