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1. http://www.mrao.cam.ac.uk/secure/amiday/talks/AMI_Day_Presentation_hogan.pdf
... Current Work Attempting to understand AGN feedback in galaxy clusters AMI Where does AMI fit in? ... Feedback needed to offset cooling and explain the deficit of cold, molecular gas in cluster cores. ... Some already observed with AMI Ideally want to observe many more (~100 150) cooling clusters in this energetically important but often overlooked frequency range. ... If bright at 1.4GHz then observe with AMI Campaign to observe many clusters at higher frequency with GISMO (2mm). ...
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Ссылки http://www.mrao.cam.ac.uk/secure/amiday/talks/AMI_Day_Presentation_hogan.pdf -- 2534.2 Кб -- 04.10.2011
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. Number . Task . Pri . Author . Created By Tool . Created On . Modified On . Completed . Modified By . Assigned To . Link To . Magic . Description
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Ссылки http://www.mrao.cam.ac.uk/~nima/_vti_pvt/_x_todo.htm -- 1.5 Кб -- 06.02.2006
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