... The spectrum of the brightest star, our Sun, shows several dark gaps perpendicular to the flow of it’s colours (figure 1). These so called spectral absorption lines where discovered in 1802 by the English scientist William Wollaston. ... Some stars as Pollux show a spectrum similar to that of our sun with strong Ca II and Fe II lines, others as Sirius or Vega show strong absorption lines of hydrogen, others, as Mira show very complicated spectra due to molecular absorption lines (see figure 5). ...

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• The Probook Project

... The described algorithm is suitable for measurements of complex images of stars. ... a) the zero-based number of stars in the complex (multicentric) image, . b) set of preliminary coordinates - x i , y i , for all stars, index i is number of a star, . ... i - index of a star in the complex image; . ... These parameters are calculated by a nonlinear method of a least squares.The main output parameters of this algorithm are x i , y i ; where the index i is number of a star in the multicentric image. ...

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... 23 Algorithm fo r evalua tion of two burn maneuv ers using linearity Input information: ( t t E1 , rEI , v t1L , t E2 2L ( ) EI )T )T ­ ­ ­ ­ the time and the state vector of initial orbit for this time ; interval of possible thrusts for transition from initial orbit to the transfer on e; the time and the state vector of the target orbit for this time ; ... We cal culate the state vector for the initial orbit for the time t1a and the target one ­ for the time t2 a . ...

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... Description . Catalog . ... In the Catalog, we publish equatorial (ЮБ 2000 , ЮД 2000 ) and galactic (l,b) coordinates of cluster centers derived as the position of overdensity in 2MASS catalog (Koposov et al. ... Distances, color-excesses and ages are the mean-square values calculated using all available evaluations from different color-magnitude diagrams. ... There are individual pages for every cluster where all available plots and parameters are published. ... 2002). ...

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The Second U.S. Naval Observatory CCD Astrograph Catalog ( UCAC2 ) Table of Contents 1) Introduction 2) Summary of the Project a) Observations and Instrumentation b) Reductions of UCAC Observations c) Computation of Proper Motions 3) Properties of the Catalog and Important Notes For the User a) Sky Coverage b) Completeness c) Positions, Proper Motions and Error Calculations d) UCAC2 Magnitudes e) 2MASS Photometry f) Non-stellar ... All stars in the UCAC2 have proper motions. ...

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• http://www.simfov.ru/catalogs/npm1/npm1.txt

Warning : date() [ function.date ]: It is not safe to rely on the system's timezone settings. You are *required* to use the date.timezone setting or the date_default_timezone_set() function. In case you used any of those methods and you are still getting this warning, you most likely misspelled the timezone identifier. We selected 'America/New_York' for 'EST/-5.0/no DST' instead in /home/photofo/public_html/space/wp-includes/functions.php on line 136 . ...

130. http://kcor.sai.msu.ru/arXiv1002.2360.pdf

131. ОТДЕЛ КОСМОЛОГИИ И ТЕОРЕТИЧЕСКОЙ АСТРОФИЗИКИ АСТРОКОСМИЧЕСКОГО ЦЕНТРА ФИАН

132. http://www.gpad.ac.ru/collaborations/gao/wv_solphys.pdf

133. ASTROSIB FFC-14, 16, 20 Field flattener-corrector

134. F-22 Raptor Airshow Demo at Langley Air Force Base

135. PENTAR: Редуктор фокуса CCD f/3.3/Field Flattener and Variable T-Adapter

136. СМ5 : Команды менеджера библиотек ACCEL Library Executive

137. http://www.sai.msu.su/gcvs/gcvs/nl74/readme

138. The Sunspot Observer - The solar regions - The description of the solar regions

139. Отдел гравитационных измерений ГАИШ