Astronet Поиск по астрономическим сайтам English Russian
       
        Точная форма слов   О проекте   Сайты   Справка
Поиск по:www.sai.msu.su/    - Поискать по всем серверам
Найдено документов: 1112 ---- Время поиска: 0.32сек.   
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

    • Пред. | 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | След.

    21. APOD: October 18, 1999 - NGC 3603: An Active Star Cluster
    ... ISAAC , VLT , ESO . Explanation: NGC 3603 is home to a massive star cluster, thick dust pillars, and a star about to explode . ...
    [ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap991018.html -- 4.7 Кб -- 02.10.2012
    Похожие документы

    22. APOD Index - Stars: Neutron Stars
    ... Explanation: How massive can a star get without imploding into a black hole? ... that the object is a neutron star of typical mass, some previous theories of neutron ...
    [ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/neutron_stars.html -- 10.6 Кб -- 21.12.2007
    Похожие документы

    23. APOD: 2003 March 14 - DEM L71: When Small Stars Explode
    ... Explanation: Large, massive stars end their furious lives in spectacular supernova explosions -- but small, low mass stars may ...
    [ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap030314.html -- 5.2 Кб -- 01.10.2012
    Похожие документы

    24. APOD: June 20, 1997 - NGC1850: Star Cluster in the LMC
    ... The white stars are massive, hotter, and younger, about 4 million years old. ... Massive stars which formed in the older main cluster have long since disappeared ... from now a similar fate awaits the massive stars of the younger cluster - burning ...
    [ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap970620.html -- 4.6 Кб -- 02.10.2012
    Похожие документы

    25. APOD: 2000 July 29 - NGC1850: Star Cluster in the LMC
    ... The white stars are massive, hotter, and younger, about 4 million years old. ... Massive stars which formed in the older main cluster have long since disappeared ... from now a similar fate awaits the massive stars of the younger cluster - burning ...
    [ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap000729.html -- 4.7 Кб -- 01.10.2012
    Похожие документы

    26. APOD: 2003 August 8 - Blue Stragglers in NGC 6397
    ... NGC 6397's massive stars have long since evolved off the main sequence , exhausting ... leave the cluster with only old low mass stars; faint red main sequence stars and ...
    [ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap030808.html -- 5.8 Кб -- 02.10.2012
    Похожие документы

    27. APOD: 2000 June 22 - Blue Stragglers In NGC 6397
    ... NGC 6397's massive stars have long since evolved off the main sequence, exhausting ... leave the cluster with only old low mass stars; faint red main sequence stars and ...
    [ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap000622.html -- 5.0 Кб -- 01.10.2012
    Похожие документы

    28. APOD: 2003 June 12 - Cyg X-1: Can Black Holes Form in the Dark?
    ... black hole from the collapsing core of a massive star is thought to be heralded by a ... X-1 , was born when a massive star collapsed -- without any supernova explosion at ...
    [ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap030612.html -- 5.4 Кб -- 02.10.2012
    Похожие документы

    29. APOD: 2005 April 2 - Cyg X-1: Can Black Holes Form in the Dark?
    ... black hole from the collapsing core of a massive star is thought to be heralded by a ... X-1 , was born when a massive star collapsed -- without any supernova explosion at ...
    [ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap050402.html -- 5.3 Кб -- 02.10.2012
    Похожие документы

    30. APOD Index - Stars: Binary Stars
    ... In a binary system, the higher mass star will evolve faster and will eventually become a compact object - either a white dwarf ... When the lower mass star later evolves into an expansion phase, it may be so close to the compact star that its outer ...
    [ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/binary_stars.html -- 8.3 Кб -- 21.12.2007
    Похожие документы

    Пред. | 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | След.

    Rambler's Top100 RFBR Яндекс цитирования