|COOKIES: By using this website you agree that we can place Google Analytics Cookies on your device for performance monitoring.|
The state and mass of H2 in starbursts: a new emerging view in the age of ALMA
If you have a question about this talk, please contact David Titterington.
I will be briefly reviewing our past views on the molecular gas in galaxies, its state and mass, and how we acquired them. Then a new potentially very different emerging view will be detailed. This was ushered by a larger ground-based survey of high-J CO and HCN lines of local merger/starburst galaxies, now augmented by very high-J CO Spectral Line Energy Distributions (SLEDs) from Herschel. I will conclude by unfolding this picture across cosmic epoch, and its utility in the age of ALMA , as well as SKA and its precursors.
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 listsAre there too may people? A head-to-head debate on overpopulation Geophysical and Environmental Processes (DAMTP/BPI) Centre of International Studies Lectures and Events
Other talksCannabis and psychosis: What are the links? Production Processes Group Seminar - 'Manufacturing at twice the speed: limits to DoD inkjet printing' Balancing forces during mitosis: from molecular motors up to tissue mechanics Unveiling the world? Aerial photographs and the social sciences in interwar France Comparative aspects of canine cancer and therapy Noise sensitivity in bootstrap percolation