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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 listsDanby Society Ivory Tower Society, Pembroke College Collective Phenomena group meeting
Other talksVibration based structural health monitoring: from Bridges to Wind Turbines What people talk about when they talk about genomes Measuring attention in rodent models of schizophrenia The origin and evolution of Homo sapiens 'A Brief History of Demons: Encounters with the Supernatural in Body and Soul' 'The German Heraclitus: Exploring the esoteric habitus of Oswald Spengler'