Astronet Поиск по астрономическим сайтам English Russian
       
        Точная форма слов   О проекте   Сайты   Справка
Поиск по:xmm.vilspa.esa.es/    - Поискать по всем серверам
Найдено документов: 54 ---- Время поиска: 0.38сек.   
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 | След.

    21. Background: motivation for developing this procedure
    ... This is particularly interesting for timing studies of isolated neutron stars, X-ray Binaries and other variable objects, such as magnetic CVs, with very soft spectra. ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/6.5.0/doc/epreject/node7.html -- 5.2 Кб -- 15.08.2005
    Похожие документы

    22. Background: motivation for developing this procedure
    ... This is particularly interesting for timing studies of isolated neutron stars, X-ray Binaries and other variable objects, such as magnetic CVs, with very soft spectra. ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/7.0.0/doc/epreject/node7.html -- 5.3 Кб -- 28.06.2006
    Похожие документы

    23. Background: motivation for developing this procedure
    ... This is particularly interesting for timing studies of isolated neutron stars, X-ray Binaries and other variable objects, such as magnetic CVs, with very soft spectra. ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/7.1.0/doc/epreject/node9.html -- 5.2 Кб -- 15.11.2007
    Похожие документы

    24. Background: motivation for developing this procedure
    ... This is particularly interesting for timing studies of isolated neutron stars, X-ray Binaries and other variable objects, such as magnetic CVs, with very soft spectra. ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/epreject/node7.html -- 5.2 Кб -- 01.07.2008
    Похожие документы

    25. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200302/fhaberl040203.pdf
    ... response The energy scale Au-edge, O-edge (BL Lacs) Emission lines (N132D and 1E0102) Vela SNR Long-term stability Internal cal source Isolated neutron stars Energy shift at Au- and O-edge Au-edge (SW mode) Average 0.995 +- 0.001 O-edge (SW mode) SNRs ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200302/fhaberl040203.pdf -- 1313.9 Кб -- 14.05.2014
    Похожие документы

    26. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200605/VBurwitz.pdf
    ... of photon spectra EU V E Vadim Burwitz EPIC CAL/OPS, MPE May 4, 2006 RX J1856.5­3754: A `stable` neutron star Individual fits with all parameters free: Simultaneous fits with NH linked: Model: tbabs*bbody from Frank Haberl Vadim Burwitz EPIC CAL/OPS, MPE ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200605/VBurwitz.pdf -- 1189.5 Кб -- 14.05.2014
    Похожие документы

    27. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200610/Burwitz.pdf
    ... 2006 Comparison of photon spectra EUVE Vadim Burwitz EPIC Calibration Meeting, October 27, 2006 RX J1856.5­3754: A `stable` neutron star Individual fits with all parameters free: Simultaneous fits with NH linked: Model: tbabs*bbody from Frank Haberl Vadim ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200610/Burwitz.pdf -- 812.0 Кб -- 14.05.2014
    Похожие документы

    28. XMM-Newton Trainee Project 2004
    ... The pulsar, a spinning neutron star with a period of only 33ms, has been observed over nearly all energy bands. ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_links/trainee/2004/gabi.shtml -- 16.0 Кб -- 13.04.2016
    Похожие документы

    29. XMM-Newton Trainee Project 2004
    ... During operations, the emphasis shifts to understanding exactly how well the instruments perform in order to reveal as clearly as possible the physics of the sun and stars, neutron stars or black holes, or galaxies at large within the universe. ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_links/trainee/2004/tutors.shtml -- 17.0 Кб -- 13.04.2016
    Похожие документы

    30. XMM-Newton Trainee Project 2005
    ... During operations, the emphasis shifts to understanding exactly how well the instruments perform in order to reveal as clearly as possible the physics of the sun and stars, neutron stars or black holes, or galaxies at large within the universe. ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_links/trainee/2005/tutors.shtml -- 17.5 Кб -- 13.04.2016
    Похожие документы

    Пред. | 1 | 2 | 3 | 4 | 5 | 6 | След.

    Rambler's Top100 RFBR Яндекс цитирования