Download Izmccd (~2.7 MB). Solution of problems at identification of star field. ... 2) Scale is not correct. ... In this case algorithm of identification will revise all values of scale from twice smaller up to twice greater. ... There should be more than value of the field "Number of stars in frame". ... The star field is considered identified if number of the identified stars more or equally to this value. It is necessary to set value from 4 up to value of field "Number of stars in frame". ...

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... Structure of Data . ... Catalog . ... In SAI OCL Catalog, we introduce our work on investigation of the Milky Way system of open star clusters. The main goal of our study is a search for new clusters using huge surveys. 168 new clusters have been already discovered by us using J,H,Ks data from 2MASS point source catalog. ... For 141 new clusters, we found their physical parameters using J,H,Ks data from 2MASS catalog and, for a number of clusters, our UBVRI CCD observational magnitudes. ...

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• SAI OCL Catalog Structure

Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...

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• The NMW survey homepage

... Three energetic mechanisms are considered: multiple supernova explosions (SNe), a hypernova explosion associated with a gamma ray burst (GRB), and the vertical impact of a high velocity cloud (HVC). ... As a consequence, multiple SNe form rings with a high ring-to-center contrast K < 100 in the HI column density, whereas single hypernova explosions form rings with K < 10. ... Our simulations show (see Fig. 6) that both multiple SNe and single hypernovae may form rings of up to 2 kpc in diameter. ...

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• Vladimir Marsakov Abstracts
• Population of Galactic globular clusters, tabl
• Anomalous Absorption Theory

... Pulkovo Astrometric Observations of Bodies in the Solar System from 1898 to 2005: Observational Database T. P. Kiseleva and E. V. Khrutskaya Pulkovo Astronomical Observatory, Russian Academy of Sciences, Pulkovskoe sh. ... The long-term work resulted in long, homogeneous series of observations of various bodies in the Solar System: Venus, Mars, Jupiter, Saturn, Uranus, Neptune, Pluto; the satellites of Mars, Jupiter, and Saturn; selected minor planets, asteroids, and comets. ... 2001; Kiseleva et al...

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• Evgenia Khrutskaya
• The Pul-3 astrometric catalogue (Second edition). Data access form.
• The Pul_ERS astrometric catalogue. Data access form

... The author attempts to approach the problem from the positions of systems analysis with account for the ideological grounds and history of space activities in Russia and abroad, comparing its current interpretation with the initial goals posed by leading theoreticians and practitioners who stood at the cradle of the space exploration era. ... The space systems recognized in Russia as priority projects are largely developed with violations of the systems approach principles. ...

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... CERN, ESA and ESO Launch "Physics On Stage" [1] . ... Beginning in February 2000, three major European research organisations are organising a unique Europe-wide programme to raise the public awareness of physics and related sciences. Physics on Stage" is launched by the European Laboratory for Particle Physics (CERN), the European Space Agency (ESA) and the European Southern Observatory (ESO), with support from the European Union. ... Physics on Stage" in 22 European Countries . ...

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• ПРИЛОЖЕНИЕ ј2 к Выпуску N2(16), март-апрель 1998

... 73P/Швассмана-Вахмана 3 . Комета 73P/Швассмана-Вахмана 3 . ... Комета 73P/Швассмана-Вахмана 3 и туманность М57 . ... Телескоп Хаббл и 73P/Швассмана-Вахмана 3 . Комета 73P/Швассмана-Вахмана 3 и М13 . ... Фрагмент С кометы 73P/Швассмана-Вахмана 3 . ... Фрагмент С Кометы 73P/Швассмана-Вахмана 3 . ... Комета McNaught - самая яркая комета 21 века . 12 января 2007 Комета McNaught - самая яркая комета . Комета McNaught - самая яркая комета южного полушария 21 века . ...

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RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . Support of activities at the Radio telescope General information Main characteristics of the Radio telescope Observing programs General view of the antenna array Main research areas Principle of generation of radio images Radio telescope 's beam Receiving systems Main characteristics of the base receiving-recording complex Calibrations Data archive and databases Publication of ... 9.4 GHz band. ...

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• Radioastrophysical department ISTP RAS SB

. ИЗГОТОВЛЕНИЕ . АСТРОНОМИЧЕСКИХ ПРИБОРОВ И ОПТИКИ . ДЛЯ ЛЮБИТЕЛЕЙ И ПРОФЕССИОНАЛОВ . FABRICATION . OF ASTRONOMICAL INSTRUMENTS AND OPTICS . FOR AMATEURS AND PROFESSIONALS . о компании . оптика . телескопы . контакт . 300 мм телескоп Ньютона на установке Добсона . about company . optics . telescope . contact . Тел./Факс.536-89-22 .

120. http://www.abitu.ru/en2002/closed/viewwork.html?work=102