... and motion of stars above and below the galactic plane imply a non luminous mass in ... kinds are due to the mass of a lensing galaxy cluster, galaxy, or compact object ...
... The anisotropic components that are of essential interest are (i) The Galactic dust emission which becomes signi cant at high frequencies (typically > 100 GHz); (ii) The Galactic thermal (free-free) emission and non-thermal (synchrotron) radiation which ...
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Ссылки http://www.mrao.cam.ac.uk/~anthony/capetown_paper/lasenby.ps -- 1071.4 Кб -- 01.05.2002 Похожие документы
... Where cores are clustered, we will also compare the velocity dispersion between cores, a simple measurable quantity that can be compared with both star formation simulations and young clusters of premain-sequence stars (e.g., Belloche et al. ...
... The main foreground components are expected to be Galactic dust, free--free and synchrotron emission as well as the kinetic and thermal SZ effects from galaxy clusters. ...
... PARAMETRIC VISIBILITIES OF SUPERMASSIVE BLACK-HOLES Active Galactic Nuclei (hereafter AGN) are galactic nuclei powered by non-stellar energy production. ...
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Ссылки http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/spie7013-172-c.pdf -- 273.0 Кб -- 20.02.2013 Похожие документы
... of three cold regions above and below the galactic plane over a period of 4.5 hours ... HI intensity mapping, HI absorption, Galactic foreground polarimetry and searches ...
... Numerous observations of galactic and extragalactic sources in the lines given above ... or the [CII] line both in galactic sources (star formations regions) and external ...
... Numerous observations of galactic and extragalactic sources in the lines given above ... CII] 158 Їm line both in galactic sources (star formations regions) and external ...
... with peculiar morphologies, especially those showing tidal tails or galactic bridges ... When complete, it will cover most of the Northern Galactic Hemisphere. ... are, for example, on average more luminous in rich clusters (MbJ = -20.07 ± 0.07, De ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2004/sloan-interacting-gals-P1.pdf -- 951.0 Кб -- 25.11.2009 Похожие документы
... size, in large-scale unbiased surveys of galactic and extra-galactic regions ... and excitation in the gaseous material of both galactic and extra-galactic sources ... galactic disks, starburst and Seyfert galaxies, and interacting galaxy systems ...