... HI in the Galaxy . JM Dickey, FJ Lockman . 28:215-61 . The Cosmic Far Ultraviolet Background . S Bowyer . 29:59-88 . ... S Bowyer . 29:59-88 . Ultraviolet Background Radiation . RC Henry . 29:89-127 . Chemical Evolution of the Galaxy . ...
... of nuclear activity are (not all present always): compact, very bright centers, Rnucl 3pc spectra with strong emission lines ultraviolet-excess X-ray emission jets and double radio sources with Rjet ~ kpc -Mpc variability over the whole spectrum on short ...
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Ссылки http://lnfm1.sai.msu.ru/~rastor/Ralf_Bender/imprs_chapter_12_2007_active_galaxies.pdf -- 2885.6 Кб -- 03.03.2008 Похожие документы
... H from hot stars can increase the Ca H line equivalent width compared to the Ca K line (Rose 1985), (b) near-ultraviolet ( NU V - V ) colors, and (c) a tendency for progressively younger ages to be inferred from increasingly higher-order Balmer lines ...
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Ссылки http://lnfm1.sai.msu.ru/~rastor/Books/Brodie&Strader_ARAA-ExtragalGC.pdf -- 1050.9 Кб -- 11.05.2010 Похожие документы