Astronet Поиск по астрономическим сайтам English Russian
       
        Точная форма слов   О проекте   Сайты   Справка
Поиск по:www.mso.anu.edu.au/    - Поискать по всем серверам
Найдено документов: 63 ---- Время поиска: 0.28сек.   
Каталог астрономических ресурсов

  • Наблюдения, инструменты и базы данных
  • Астрометрия и служба времени
  • Небесная механика и гравиметрия
  • Теоретическая астрофизика
  • Солнечная система
    		•
  • Звезды
  • Галактики, квазары, космология
  • Исследование космоса
  • Общие вопросы
  • Прочее

    • 1 | 2 | 3 | 4 | 5 | 6 | 7 | След.

    1. http://www.mso.anu.edu.au/~raquel/GRC_poster_5.pdf
    ... We present the vertical structure and linear growth of the MRI in a weakly ionized, stratified protostellar disk, assuming dust grains are well mixed with the fluid. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~raquel/GRC_poster_5.pdf -- 1425.4 Кб -- 13.09.2007
    Похожие документы

    2. http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/Bizyaev04
    ... disk is very thin, we assume that its inclination angle is 90 .For all other ... for the stellar disk in R. This can be explained by stronger dust extinction in the ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/Bizyaev04 -- 2057.9 Кб -- 09.07.2007
    Похожие документы

    3. http://www.mso.anu.edu.au/~charley/papers/LHBASSC2008.pdf
    ... formed by accretion from the dust, planetesimals and planetary embryos in a protoplanetary disk during a 90 million year period ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/LHBASSC2008.pdf -- 856.7 Кб -- 08.02.2009
    Похожие документы

    4. http://www.mso.anu.edu.au/seminars/abstracts/20141219-1400.html
    ... The properties of the midplanes of planet-forming protostellar disks remain largely unprobed by observations due to the high optical depth of dust and commonly observed molecules. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20141219-1400.html -- 4.5 Кб -- 10.04.2016
    Похожие документы

    5. http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/Gerhard02
    ... Luminosity distribution of the bulge and disk Because of the strong dust obscuration by the intervening disk, the structure of the inner Galaxy is best analyzed in the NIR. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/Gerhard02 -- 285.1 Кб -- 13.05.2006
    Похожие документы

    6. http://www.mso.anu.edu.au/pfrancis/roleplay/newstarform.pdf
    ... Curiously, most of these stars were surrounded by spinning disks of gas and dust, about 1013 metres across. 1 What does this mean? ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/newstarform.pdf -- 58.2 Кб -- 15.04.2004
    Похожие документы

    7. http://www.mso.anu.edu.au/~kcf/surya/misc_papers/Kassin06
    ... In doing this, we ignore radial dust gradients in the disk and the fact that dust reddening is likely to b e large for the ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/misc_papers/Kassin06 -- 1071.2 Кб -- 24.05.2006
    Похожие документы

    8. http://www.mso.anu.edu.au/~brian/A3002/lecture1_last_a.pdf
    ... NGC 2997 Face on view З We live at edge of disk З Disadvantage: structure obscured by "dust". ... disk Bulge = 1010 M The Dark Halo M BH = 109 M = 1012 M M DH Stellar populations: summary З The Milky Way thus has at least ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~brian/A3002/lecture1_last_a.pdf -- 920.8 Кб -- 15.09.2008
    Похожие документы

    9. Raquel Salmeron - Research Interests and Experience
    ... is a fundamental topic, because this instability is the leading mechanism to generate MHD turbulence within the disk and, as such, it measures the ability of the magnetic field to remove angular momentum from the disk material so accretion can proceed ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~raquel/interests2.html -- 7.8 Кб -- 01.10.2012
    Похожие документы

    10. Untitled
    ... The ratio of the polarization and colour during these changes resembled that of interstellar dust suggesting a dusty disk around the star. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~bessell/research.html -- 39.3 Кб -- 01.10.2012
    Похожие документы

    1 | 2 | 3 | 4 | 5 | 6 | 7 | След.

    Rambler's Top100 RFBR Яндекс цитирования