Astronet Поиск по астрономическим сайтам English Russian
       
        Точная форма слов   О проекте   Сайты   Справка
Поиск по:hea-www.harvard.edu/    - Поискать по всем серверам
Найдено документов: 780 ---- Время поиска: 1.18сек.   
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. | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14 | 15 | 16 | След.

    101. ECT: Time Warp
    ... Why doesn't it say that the Sun rises at 5 p.m. for them? Can the Sun possibly rise for them at the very same moment it does for us? ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/ECT/Warp/warp.html -- 19.9 Кб -- 01.10.2012
    Похожие документы

    102. http://hea-www.harvard.edu/~kim/pap/2013_GCLMXB_obs.pdf
    ... Following Sivakoff et al. (2007), the stellar encounter rate can be written as M 1.5 GC r -2.5 h , where MGC and rh are the GC mass and the half-mass radius. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2013_GCLMXB_obs.pdf -- 656.0 Кб -- 24.04.2013
    Похожие документы

    103. http://hea-www.harvard.edu/~kim/pap/2004_champo.pdf
    ... been to use single-slit (FLWO 1.5 m with FAST) spectroscopy for isolated r 0 < 17 ... Barden et al. 1994) on the WIYN 3.5 m and CTIO 4 m telescopes enables us to acquire ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2004_champo.pdf -- 1732.7 Кб -- 06.12.2010
    Похожие документы

    104. http://hea-www.harvard.edu/~kim/pap/2004_XLF.pdf
    ... 5 ф 1:6) ; 1038 ergs sю1 (with an error at 90%), which may be consistent with the Eddington luminosity of neutron stars with ... This break could also correspond to the Eddington luminosity of a $3.5 M accreting black hole. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2004_XLF.pdf -- 361.1 Кб -- 06.12.2010
    Похожие документы

    105. http://hea-www.harvard.edu/QEDT/Papers/3c351_new.ps
    ... The corresponding mass loss rate is 0:05 ! — M ! 5 M fi yr \Gamma1 for covering factors between 1% and unity. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/QEDT/Papers/3c351_new.ps -- 219.2 Кб -- 21.06.1994
    Похожие документы

    106. http://hea-www.harvard.edu/ECT/pdf/Warp.pdf
    ... Why doesn't it say that the Sun rises at 5 p.m. for them? Can the Sun possibly rise for them at the very same moment it does for us? ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/ECT/pdf/Warp.pdf -- 142.5 Кб -- 21.01.1999
    Похожие документы

    107. http://hea-www.harvard.edu/~pgreen/Papers/aox_composites98.pdf
    ... Follow-up (6 х10 с resolution) optical spectra with S/N B 10 (in the continuum at D4500 с) were obtained at the Multiple Mirror Telescope (MMT) and the 2.5 m duPont telescope. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/aox_composites98.pdf -- 594.3 Кб -- 19.09.2005
    Похожие документы

    108. http://hea-www.harvard.edu/~pgreen/Papers/aox_composites98.ps
    ... Follow­up (6х10 resolution) optical spectra with с S/NB 10 (in the continuum at D4500 were obtained at с) the Multiple Mirror Telescope (MMT) and the 2.5 m duPont telescope. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/aox_composites98.ps -- 1408.7 Кб -- 19.09.2005
    Похожие документы

    109. http://hea-www.harvard.edu/~bradw/cv/papers/hsiSPIE.pdf
    ... The individual channels are nominally 8 1 pm diameter (yielding an 80 : 1 LID ratio) arranged in a hexagonal close-packed structure with 10 1 pm (typically 9.5 m) channel-to-channel spacing. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~bradw/cv/papers/hsiSPIE.pdf -- 529.4 Кб -- 02.01.2014
    Похожие документы

    110. http://hea-www.harvard.edu/~kim/pap/2008_N7619.pdf
    ... Taking the mass-loss rate from Faber & Gallagher (1976), we estimate the accumulated mass from stellar mass loss over the Hubble time to be 1:5 ; 1010 M , which is comparable to the total mass of the hot gas in the core-tail structure (2 ; 1010 M ). ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2008_N7619.pdf -- 724.0 Кб -- 06.12.2010
    Похожие документы

    [ В начало ] Пред. | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14 | 15 | 16 | След.

    Rambler's Top100 RFBR Яндекс цитирования