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    71. http://www.mrao.cam.ac.uk/yerac/thoraval/thoraval.ps
    ... in the spatial dis­ tribution of the dust would have important consequences for the modelling of molecular clouds because the UV light penetration and therefore the physical and chemical processes depend strongly on their structure (cf Boiss'e (1990 ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/yerac/thoraval/thoraval.ps -- 1130.5 Кб -- 22.02.1995
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    72. Galactic SNRs: Documentation
    ... 2.3.1 Radio . 2.3.1 UV/Optical/Infra-red . 2.3.3 X-ray . 2.3.4 Other . 2.4 Questionable SNRs listed in the catalogue . ... SNRs by Koo & Heiles (1991); and the catalogue by Fesen & Hurford (1996) of UV/optical/infra-red lines identified in SNRs ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/projects/surveys/snrs-2004/snrs.info.html -- 60.5 Кб -- 10.04.2016
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    73. Galactic SNRs: Documentation
    ... 2.3.1 Radio . 2.3.2 UV/Optical/Infra-red . 2.3.3 X-ray/ -ray . 2.3.4 Other . 2.4 Questionable SNRs listed in the catalogue . ... SNRs by Reach et al. (2006); and the catalogue by Fesen & Hurford (1996) of UV/optical/infra-red lines identified in SNRs ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/projects/surveys/snrs-2006/snrs.info.html -- 71.4 Кб -- 10.04.2016
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    74. http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/spie7013-144.pdf
    ... 4.2 Influence of the uv coverage As Fig. 5 demonstrates, the 15 telescope uv coverage gives nearly perfect images, and point ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/spie7013-144.pdf -- 830.0 Кб -- 20.02.2013
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    75. http://www.mrao.cam.ac.uk/~bn204/publications/2010/N6946.pdf
    ... Since the uv coverage of the AMI-LA varies across the frequency channels we quantified the amount of flux lost in each channel relative to channel 4 by sampling the total power 8.5 GHz map to match the uv coverage in each of the AMI-LA frequency channels. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/publications/2010/N6946.pdf -- 317.0 Кб -- 10.08.2012
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    76. G189.1+3.0
    ... Mufson et al. 1986, AJ, 92, 1349. Radio, IR, optical, UV and X-ray comparison, including VLA at 1.6 GHz (3".8?3".3 and 40''). ADS . Petre et al. ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/projects/surveys/snrs/snrs.G189.1+3.0.html -- 13.6 Кб -- 10.04.2016
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    77. The distant DRAGNs survey
    ... Alignment effect: The UV, optical and IR emission from high- radio galaxies tends to ... used where needed to fill in short uv spacings and allow valid spectral comparisons ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/yerac/lawgreen/lawgreen.html -- 23.0 Кб -- 08.12.2003
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    78. Galactic SNRs: Documentation
    ... 2.3.1 Radio . 2.3.2 UV/Optical/Infra-red . 2.3.3 X-ray/ -ray . 2.3.4 Other . 2.4 Questionable SNRs listed in the catalogue . ... SNRs by Reach et al. (2006); and the catalogue by Fesen & Hurford (1996) of UV/optical/infra-red lines identified in SNRs ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/projects/surveys/snrs-2009/snrs.info.html -- 86.5 Кб -- 02.09.2014
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    79. http://www.mrao.cam.ac.uk/yerac/lawgreen/lawgreen.ps
    ... speed or density. ffl Alignment effect: The UV, optical and IR emission from high­z ... used where needed to fill in short uv spacings and allow valid spectral comparisons ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/yerac/lawgreen/lawgreen.ps -- 213.1 Кб -- 22.02.1995
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    80. http://www.mrao.cam.ac.uk/yerac/gueth/gueth.ps
    ... which guarantees some homogeneity in terms of uv coverage and noise level (see, for ... techniques, which seem to need a better uv coverage than the one available with the ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/yerac/gueth/gueth.ps -- 309.0 Кб -- 22.02.1995
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