... Elena Seifina and Lev Titarchuk "On the nature of the compact object in SS433: observational evidence of X-ray photon index saturation" 2010, Astrophysical. ... A.M. Cherepashchuk, R.A. Sunyaev, E.V. Seifina, E.A. Antokhina, D.I. Kosenko, S.V. Molkov, N.I. Shakura, K.A. Postnov, A.N. Timokhin, I.E. Panchenko "INTEGRAL Observations of SS433: Analysis of Precessional and Orbital X-ray Periodicities" 2007, 6th INTEGRAL Workshop, Eds. S. Grebenev, R.A. Sunyaev, p.411 (astro-ph/0610235) . ...
... NASA Main Page . NASA Organizations Index . ... Marshall Space Flight Center . ... Science @ NASA: news . ... Goddard Space Flight Center: Science missions . National Space Science Data Center . data from NASA space flight missions, . ... High Energy Astrophysics Science Research Center (HEASARC) - a source of gamma-ray, X-ray, extreme ultraviolet, other wavebands observations of cosmic (non-solar) sources. ... Kennedy Space Center - Publisher's Photo Corner - Photograph Index . ...
... Cloud" CALDWELL 14 MESSIER 34 MESSIER 45 CALDWELL 41 DEEPSKY "Large Mag. Cloud MESSIER 79 MESSIER 38 MESSIER 42 MESSIER 36 MESSIER 37 MESSIER 35 SAO 234480 MESSIER 41 MESSIER 44 CALDWELL 53 CALDWELL 92 NGC 3377 CALDWELL 91 NGC 4261 MESSIER 68 CONSTELLATION Coma Berenices CALDWELL 99 CALDWELL 94 CALDWELL 77 CALDWELL 80 MESSIER 51 MESSIER 04 MESSIER 13 MESSIER 92 MESSIER 06 MESSIER 07 MESSIER 08 ... This is" "short for 'Quasi stellar objects.' ...
... Страна-разработчик МКА США (фирма Spectrum Astro)2. Назначение МКА Экспериментальный испытательный МКА военного назначения (отработка технологий для распределенных апертур)3. Количество МКА в системе Одиночный запуск4. Год запуска МКА 19.07.2000 г.5. Срок активного существования МКА 1 год6. Баллистические характеристики МКА Высота орбиты 550 км7. ... Обеспечивает выведение на орбиту двух неуправляемых, оснащенных радиоаппаратурой малой мощности пикоспутников массой далее . ...
. Ecliptic (Greek - eclipse) is a big circle of the celestial sphere with a yearly visible Sun's movement. It is crossed with the celestial equator in the points of vernal and autamnal equinox. The ecliptic plane is bent to the plane of the celestial equator with the angle 23° 27'. Back .
... SB, Porb = 55.9212d. V0745 Cas| ... Component B of the double system observed brighter than in the Hipparcos Input Catalogue. ... The variability may be due to the fainter component. ... Type ELL: is also possible. pi Cas| ... Variability type and spectral type (F2/F3Ib/II) do not agree. ... Variability type and spectral type (F3/F5II) do not agree. ... Variability may be due to component B. VZ Pic| ... Variability may be due to component B. V1377 Ori| ... SB, Porb = 9.073d. V0421 Cep|105091| ...
... РЕШЕНИЕ ЗАДАЧ СФЕРИЧЕСКОЙ АСТРОНОМИИ . ... Оценка условий наблюдения солнечных и лунных затмений . ... Для наблюдателей, находящихся в различных точках земной поверхности, моменты контактов дисков Солнца и Луны происходят в разные моменты времени, по мере движения лунной тени. Характерные фазы затмения Луны видны всеми наблюдателями одновременно, что часто использовалось в прошлом для определения долгот географических пунктов. ... Такие данные содержатся на многих серверах сети Интернет. ...
... Now comes a remarkable opportunity for all AAAP members to learn more about our closest star-- straight from a leading figure in solar physics and expert on solar eclipses. Dr. Fred Espenak from the NASA Goddard Spaceflight Center will present Predicting and Chasing Solar Eclipses at a special lecture on March 30. ... Information about future solar eclipses visible from Princeton will be distributed at this event, at which the public is also welcome (bring your kids too!) ...
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Ссылки http://www.princetonastronomy.org/newsletters/03_2007sidereal.pdf -- 357.4 Кб -- 10.03.2007 Похожие документы
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