Sternberg Astronomical Institute (Moscow University)

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• Sternberg Astronomical Institute — The Sternberg Astronomical Institute (Государственный астрономический институт имени Штернберга in Russian), also known as GAISh (ГАИШ), is a research institution in Moscow, Russia, a division of Moscow State University. The institute is named… …   Wikipedia

• Moscow State University — MGU redirects here. For other uses, see MGU (disambiguation). Moscow University redirects here. For the tanker, see MV Moscow University. Lomonosov Moscow State University Московский государственный университет имени М. В. Ломоносова Coat of arms …   Wikipedia

• Lomonosov Moscow State University — Infobox University name = M. V. Lomonosov Moscow State University established = 1755 city = Moscow, Russia native name = Московский государственный университет имени М. В. Ломоносова image size = 200px caption = Moscow State University s main… …   Wikipedia

• Supernova — This article is about the astronomical event. For other uses, see Supernova (disambiguation). Multiwavelength X ray, infrared, and optical compilation image of Kepler s supernova remnant, SN 1604. A supernova is a stellar explosion that is more… …   Wikipedia

• New Catalogue of Suspected Variable Stars — The New Catalogue of Suspected Variable Stars (NSV) is a star catalogue containing 14,811 stars which, although suspected to be variable, were not given variable star designations prior to 1980. It was published in 1982.[1] References ^ New… …   Wikipedia

• Nikolai Shakura — Nikolai Ivanovich Shakura (Николай Иванович Шакура) was born in Belarus SSR on October 7, 1945. He is the head of the relativistic astrophysics department at the Sternberg Astronomical Institute, Moscow University. A well known specialist in… …   Wikipedia

• Эффект «Пионера» — Иллюстрация выхода космических аппаратов за пределы Солнечной системы Эффект «Пионера» (эффект «Пионеров», аномалия «Пионеров») наблюдаемое отклонение в траектории движения …   Википедия

• Nova — For other uses, see Nova (disambiguation). Artist s conception of a white dwarf star accreting hydrogen from a larger companion A nova (plural novae) is a cataclysmic nuclear explosion in a star caused by the accretion of hydrogen on to the… …   Wikipedia

• Capella (star) — For other uses, see Capella (disambiguation). Capella Aa/Ab Capella is the brightest star in Auriga Observation data Epoch J2000.0     …   Wikipedia

• VY Большого Пса — Звезда …   Википедия

• List of most luminous stars — Below is a list of stars arranged in order of decreasing luminosity (increasing bolometric magnitude). Accurate measurement of stellar luminosities is quite difficult in practice, even when the apparent magnitude is measured accurately, for three …   Wikipedia