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ALMA studies of submm galaxies
If you have a question about this talk, please contact David Titterington.
Ultraluminous infrared galaxies have been claimed to be a significant component of the star formation at z>1. The most luminous of these galaxies are detectable as sources in the submm wavebands with instruments such as Herschel or SCUBA -2. I will discuss recent work with SCUBA -2 and ALMA to investigate the properties of this population, the physical processes driving their extreme luminosities and their relation to galaxy populations at the present day.
This talk is part of the Cavendish Astrophysics Seminars series.
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Other listsBehaviour, Ecology & Evolution Seminar Series EPRG Energy and Environment (E&E) Series Michaelmas 2011 The Yerushah Lecture 2012
Other talks13th Annual Disability Lecture - The Power of Design: inclusion or exclusion? The destabilization of capillary rafts into armored droplets Cosmic magnetism in simulations of disk galaxy formation Directed Assembly of Active Colloidal Devices A Taste for Virtue: Eighteenth-Century Epicureanism and Rousseau's Political Thought Power laws in dislocation plasticity