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    61. http://www.mrao.cam.ac.uk/~rachael/compphys/Lecture%201.pdf
    ... Fourier Transforms and Signal Processing ("Big Ben") Ordinary DEs: Trojan asteroids N-body simulations: Tidal tails of interacting galaxies Eigenvalue problems: Localization in a linear chain Abstract simulation: Percolation on a 2-D lattice ("Forest Fire ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~rachael/compphys/Lecture%201.pdf -- 912.2 Кб -- 30.10.2007
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    62. http://www.mrao.cam.ac.uk/~rachael/compphys/CompPhys2.pdf
    ... Once this is achieved we are able to begin the numerical experiment proper; for example the simulation of interacting galaxies. ... 36 Computational Physics Figure 3.4: The interacting galaxies NGC 3395 and NGC 3396. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~rachael/compphys/CompPhys2.pdf -- 866.4 Кб -- 22.10.2007
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    63. http://www.mrao.cam.ac.uk/projects/skads/lofar/talks/Beck.MKSP.Cambridge.pdf
    ... sources: polarised Galactic regions (Fan, NPS); SNR, HII & planetary nebulae as Faraday screens Nearby galaxies: spiral, barred, edge-on, dwarf, interacting, blue compact, Virgo cluster members Intergalactic filaments, e.g. in galaxy groups Polarised ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/skads/lofar/talks/Beck.MKSP.Cambridge.pdf -- 2669.6 Кб -- 07.04.2009
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    64. Astrophysics Group AMI Science
    ... Galaxy clusters grow and evolve by interacting with smaller subsystems. ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/facilities/ami/ami-science/ -- 24.8 Кб -- 10.04.2016
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    65. Galaxy Evolution: Radio sources and their environments
    ... Paul Alexander . P.Alexander@mrao.cam.ac.uk . As radio sources evolve they strongly interact with their environment. ... We are investigating how this interaction effects galaxy evolution in general as well as the feedback effect of the radio ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~pa/galaxy_evolution/science_RSenvironment.html -- 6.7 Кб -- 24.01.2002
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    66. PPT Slide
    ... HST optical image 0.8 microns . The Experiment: AGN and galaxy evolution . ... A small fraction of galaxies contain an “Active Nucleus” (AGN) ? ... interact strongly with their environment . Immense power of AGN ? ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~pa/StructureEvolution/tsld007.htm -- 2.2 Кб -- 27.08.1997
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    67. http://www.mrao.cam.ac.uk/~anthony/latex/Firmani.ps
    ... High-resolution lensing for a cluster of galaxies and the rotation curves of several dark matter dominated dwarf and LSB galaxies show evidence of shallow halo cores. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~anthony/latex/Firmani.ps -- 26.1 Кб -- 15.06.2000
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    68. Astrophysics Group Stars ? Birth and Death
    ... Cosmology . Galaxies and Quasars . Pulsars . Stars ? Birth and Death . ... Throughout our Galaxy, new generations of stars are continually being born and old ... 100 kilometres per second; further out, they interact with the surrounding cloud and ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/outreach/stars-birth-and-death/ -- 16.5 Кб -- 10.04.2016
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    69. http://www.mrao.cam.ac.uk/~bn204/phd_era/publications/kiel.pdf
    ... started a programme of observations of nearby starburst and AGN galaxies with MICHELLE, with the aim of investigating the spatial extent of "Unidentified Infrared Bands (UIB)" emission in these galaxies, and in particular relating these to multi-frequency ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/phd_era/publications/kiel.pdf -- 953.3 Кб -- 12.07.2002
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    70. http://www.mrao.cam.ac.uk/~krause/KA-nam-2006-poster.pdf
    ... galaxies at redshift > 0.5 show associated optical emission: emission lines + rest frame blue continuum, correlations of many properties are evidence for the interaction · Jet induced star formation has been suggested (confirmed by finding absorption ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~krause/KA-nam-2006-poster.pdf -- 847.4 Кб -- 31.03.2006
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