|COOKIES: By using this website you agree that we can place Google Analytics Cookies on your device for performance monitoring.|
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.
This talk is included in these lists:
Note that ex-directory lists are not shown.
Other listsCrucible/Microsoft HCI Reading Group Cambridge University International Development (CUID) MAGDALENE FESTIVAL OF SOUND
Other talksArchitectures of Law: Courts, Space and Legal Legitimacy Using Mouse Models to Understand Metastatic Spread and Tumour Heterogeneity The Anne McLaren Lecture What I saw last winter SME Growth Challenge - make your management fit for growth SAP Open Forum