... Red - 8.0 m Green - 4.5 m Blue - 3.6 m Dwarf galaxies do not have SEDs well matched by templates Infrared observations show us that even low metallicity galaxies have dust However, dust properties are different from their higher metallicity counterparts ...
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Ссылки http://www.naic.edu/~astro/hiconference/hiconf_pdfs/aohi08_rosenberg.pdf -- 2592.6 Кб -- 08.02.2008 Похожие документы
... Nominal read head position -350 m. (8) Playback the track recorded in step (6) in the forward direction, peaking the reproduce power with read track 15. ...
... ISM The propagation effects from Galactic electron-density inhomogeneities can be divided into diffractive and refractive phenomena, due respectively to small ($10^{6} н 10^{8}$ m) and large ($10^{10} н 10^{12}$ m) scales in the scattering medium ...
... The same observations serve a dual purpose, and can also be used to search for a redshifted HI emission signal, with a mass limit of a few times 10 8M . ...
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Ссылки http://www.naic.edu/vscience/schedule/tpfiles/LanetagA1709tp.ps -- 98.9 Кб -- 19.04.2004 Похожие документы