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: 236 ---- Время поиска: 0.47сек.   
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

    • [ В начало ] Пред. | 8 | 9 | 10 | 11 | 12 | 13 | 14 | 15 | 16 | 17 | След.

    111. http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/kranz01.pdf
    ... However, kinematic feedback to the gas from regions of massive star formation, from expanding gas shells produced by supernova explosions and from other sources of turbulence, introduces small-scale random noise in the velocity пelds. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/kranz01.pdf -- 2023.5 Кб -- 09.07.2007
    Похожие документы

    112. http://www.mso.anu.edu.au/~fbriggs/LOFAR_SciApp_1.0.pdf
    ... of radio supernova remnants associated with the collapse of massive stars ... total mass in baryons ­ much less mass than in stars or in the ionized intergalactic ... responsible for this emission seem clear (massive star formation, OB stars, SNe and ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~fbriggs/LOFAR_SciApp_1.0.pdf -- 1914.3 Кб -- 17.04.2003
    Похожие документы

    113. http://www.mso.anu.edu.au/~kcf/pubs_top20/100.pdf
    ... types of objects : SN Ib/c, which are probably massive stars that undergo core collapse after losing their hydrogen atmospheres ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/100.pdf -- 1358.4 Кб -- 16.10.2011
    Похожие документы

    114. Research Interests
    ... Gas is simple: we understand how it behaves. There is far more mass in gas than stars. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/html_dir/firstlight/node24.html -- 5.7 Кб -- 02.10.2012
    Похожие документы

    115. http://www.mso.anu.edu.au/seminars/abstracts/20160407-1100.html
    ... wide range of objects were discovered to emit significant amounts of energy in the high-energy gamma-ray regime, including star-forming regions, pulsars, supernova remnants, massive binaries, the diffuse interstellar medium, the Galactic Centre, AGN, etc ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20160407-1100.html -- 4.7 Кб -- 10.04.2016
    Похожие документы

    116. http://www.mso.anu.edu.au/~plah/Home_Page_Stuff/files/SKA_Forum_2010.pdf
    ... around Abell 370 appear normal; they have HI Mass to Light Ratio and a Star Formation Rate to HI Gas correlation similar to ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~plah/Home_Page_Stuff/files/SKA_Forum_2010.pdf -- 2113.2 Кб -- 28.07.2010
    Похожие документы

    117. http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/Dutton05
    ... 9 ) We obtain the baryonic mass from the observations of stars and gas in the disk ... independent of the initial mass function (IMF) and star formation (SF) history ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/Dutton05 -- 1180.7 Кб -- 21.11.2006
    Похожие документы

    118. CHIAKI's Publication List
    ... Explosive Nucleosynthesis in Massive Pop III Stars and Abundances in Metal-Poor Stars and M87 . ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~chiaki/paper.html -- 33.6 Кб -- 09.04.2016
    Похожие документы

    119. http://www.mso.anu.edu.au/seminars/abstracts/20150213-1400.html
    ... turbulence and the mass and gravity of its comprising gas and dust, a system which governs the formation of stars in the dense ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150213-1400.html -- 6.3 Кб -- 10.04.2016
    Похожие документы

    120. http://www.mso.anu.edu.au/~gdc/talks/LocalGroupLect_17Dec2012.pdf
    ... have high DARK MATTER content ­ in some dwarfs the mass/light ratio (with mass measured via the velocity dispersion of the stars or via the circular velocity of the gas) exceeds 100, while the mass-to-light ratio of the stars is typically of order unity ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~gdc/talks/LocalGroupLect_17Dec2012.pdf -- 2242.9 Кб -- 17.12.2012
    Похожие документы

    [ В начало ] Пред. | 8 | 9 | 10 | 11 | 12 | 13 | 14 | 15 | 16 | 17 | След.

    Rambler's Top100 RFBR Яндекс цитирования