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201. Amateur Astronomers Association of Princeton
... Observatory . ... THE HISTORY OF AAAP . ... After introductory remarks by Robert Sanders, founder of the Association, it was moved that the name of the organization be Amateur Astronomers Association of Princeton. ... 2/72 First issue of Sidereal Times, so named by Editor Roxanne Tobin. ... 5/72 Election of officers: Norman Sperling, Director; John Church, Assist. ... Sidereal Times, John gives the following report: . ... Sidereal Times.) ... Amateur Astronomers Association of Princeton Т? 2015. ...
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Ссылки http://www.princetonastronomy.org/history.html -- 87.0 Кб -- 23.03.2016
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202. http://site2010.sai.msu.ru/static/doc/VKornilov_Scheglov_site2010.pdf
Peter Scheglov pioneer of site testing in the Central Asia A.Tokovinin & V. Kornilov Promote astronomy iin the Promote astronomy n the Central Asia Central Asia Tashkent P..Scheglov iidentified CenttralAsiian siites wiith PScheglov dentified Cen ral Asan stes wth a llarge ffraction off cllear sky and callm attmoa arge raction o cear sky and cam a mospherre, iin colllaboration wiith metteorologists. sphe e, n colaboration wth me eorologists. ... Problems of optical astronomy). ...
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Ссылки http://site2010.sai.msu.ru/static/doc/VKornilov_Scheglov_site2010.pdf -- 2099.4 Кб -- 27.10.2010
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203. http://sn.sai.msu.ru/~sil/preprints/al534.pdf
... 32, No. 8, pp. 592603. i Central Regions of the Early-Type Galaxies in the NGC 3169 Group O. K. Sil'chenko1* and V. L. Afanasiev 1 2 Sternberg Astronomical Institute, Universitetskii pr. ... The mean age of the stellar populations in the centers of all three galaxies has been found to be approximately the same, 1 Gyr. ... In contrast, in NGC 3166, there is a metallicity gradient, but the stellar age remains approximately constant up to a distance of 8 from the center. ...
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Ссылки http://sn.sai.msu.ru/~sil/preprints/al534.pdf -- 740.1 Кб -- 04.10.2006
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204. http://www.2dfquasar.org/Papers/2002MNRAS.337..275C.pdf
... 337, 275292 (2002) The correlation of line strength with luminosity and redshift from composite quasi-stellar object spectra S. M. Croom,1 K. Rhook,1 E. A. Corbett,1 B. J. Boyle,1 H. Netzer,2 N. S. Loaring,3 L ... We measure highly significant Baldwin effects for most broad emission lines (C IV 1549, C III] 1909, Mg II 2798, H ,H ) and show that they are predominantly caused by correlations with luminosity, not redshift. ... The correlations of log W with log(1 + z ) for each line. ...
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Ссылки http://www.2dfquasar.org/Papers/2002MNRAS.337..275C.pdf -- 831.9 Кб -- 04.03.2004
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