. Main . Final stage of OC "MIR" flight . Photoarchives . RUSSIAN AVIATION AND SPACE AGENCY . CENTRAL SCIENTIFIC RESEARCH . MACHINE BUILDING INSTITUTE . MISSION CONTROL CENTER . Russian . Earth Orbiting Complex "Mir" . The material submitted to the UNO Science and Engineering Subcommittee 38 session on peaceful use of space (Vienna 12-13 Feb 2001) as an oficial UNO document . Press-conference at MCC February 28, 2001, U.N. Koptev

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... The kinematics, structure, and stellar population properties in the centers of two early-type spiral galaxies of the Leo Triplet, NGC 3627 and NGC 3623, are studied by means of integral-field spectroscopy. ... In the center of NGC 3627 we observe noticeable gas radial motions, and the stars and the ionized gas in the center of NGC 3623 demonstrate more or less stable rotation. ... In this work we consider two nearby early-type spiral galaxies belonging to the famous Leo Triplet, NGC 3623 and NGC...

... During all period of our investigations Dr. N.Sumzina from the Institute of Applied Astronomy of RAS had prepared the Numbered Minor Planet positions from MPC Database for our processing with kind permission of the Director of Minor Planet Center Prof. Braian Marsden. ... Our extensive processing of the MPC data allows us to conclude that CCD observations of the Numbered and Unnumbered Minor Planets have the errors, sometimes very crude. ...

... Смарт-1' ? первая автоматическая станция Европейского космического агентства для исследования Луны. Аппарат создан по заказу ЕКА Шведской космической корпорацией при участии почти 30 субподрядчиков из 11 европейских стран и США. ... первый аппарат в программе 'Small Missions for Advanced Research in Technology' ? ... 1М (космический аппарат) . ... 2МВ (космический аппарат) . 3МВ (космический аппарат) . ... AGILE (космический аппарат) . ... ANS (телескоп) . ... Союз (космический корабль) . ...

... Maps of six sources (0420+022, 0420-014, 1308+326, 1345+125, 1803+784, and DA 193) obtained with milliarcsecond resolution are presented and discussed, together with their broadband (1­22 GHz) spectra obtained on the RATAN­600 radio telescope at epochs close to those of the VLBI observations. ... The image (Fig. 5) shows that the source structure at 18 cm is compact, consisting of a VLBI core and two jet components, with the outer component lying 5 mas (30 pc) to the northwest of the core ( = 54 ). ...

We present a catalogue of galaxies for which spatially resolved data on their internal kinematics have been published; there is no apriori restriction regarding their morphological type. The catalogue lists the references to the articles where the data are published, as well as a coded description of these data: observed emission (E) or absorption (A) data, optical (O) or radio (R) data, velocity (V) or velocity dispersion (D), radial profile (1) or 2D field (2). ...