... based on a comprehensive dust model and relatively simple radiative transfer, and illustrate their application to objects in the near-by universe with good multi-wavelength data including some new high resolution mid-infrared imaging (NGC 520 and Arp 220 ...
... Physics Anthony Lasenby Astrophysics Group, Cavendish Laboratory, Cambridge, UK Oxford, 14 April 2008 Over view I am basically a cosmologist, interested in the Cosmic Microwave Background, and early universe Why am I here talking about `Geometric Algebra ...
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Ссылки http://www.mrao.cam.ac.uk/~anthony/oxford_undergrad_physics_conf_april_2008.pdf -- 2164.2 Кб -- 20.04.2008 Похожие документы
... The distribution of matter in the Universe and its composition is one of the most fundamental problems in astrophysics. ... There is growing evidence for the presence of non-luminous matter in the Universe. ...
... Title: Modeling the nature of the ISM in galaxies during the star formation activity peak of the Universe Abstract: At redshift z1-3 the star-formation activity of the Universe reached its peak, after which it dropped towards its current day value ...
... ae ? is the mean, comoving density of the Universe and oe(M;z) is the power spectrum as a function of the mass scale, M . ... flux density, there is an enormous difference between the number of highredshift clusters in a critical and open universe ...
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Ссылки http://www.mrao.cam.ac.uk/ppeuc/astronomy/papers/bartlett.ps -- 131.7 Кб -- 25.07.1997 Похожие документы
... 2 Should act as a check: luck vs luminosity Conclusions Blind Surveys Unbiased view of the history of cold gas in the Universe Happening now with JVLA/PdBI Happening in the near future with ALMA Will finally move out of small number statistics Results of ...
... Areas to be covered include: - AGN and Galaxy Evolution - Gas in Galaxies - The High-redshift Universe and the First Galaxies - Galaxy Assembly and Cosmic Star-formation History - Galaxy Clusters and the Role of Environment Participation will be limited ...
... Brinks ) F. Feroz Lunch (canteen) Short talks: Star forming galaxies in HI in galaxies at high J. Zwart Break the early universe redshift L. Chemin (30 mins) (Scott Chapman ) (Filipe Abdalla ) V. Coreless SKA for the user (panel session) F. Radio galaxies ...
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Ссылки http://www.mrao.cam.ac.uk/projects/skads/mcct/mcct_timetable.pdf -- 120.3 Кб -- 14.08.2008 Похожие документы