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101. http://ocl.sai.msu.ru/catalog/dat/readme/
J/AstL/vol/page SAI Open Clusters Catalog (Glushkova+, 2009) ================================================================================ Automated search for star clusters in large multiband surveys. ... Color excesses E(B-V), distance moduli and ages were determined for 141 new and 27 known, but poorly studied clusters. We present the Sternberg Astronomical Institute Open Clusters Catalog (SAI OCL Catalog) of coordinates, diameters and main physical parameters of these clusters. ...
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Ссылки http://ocl.sai.msu.ru/catalog/dat/readme/ -- 5.7 Кб -- 01.10.2012
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102. Why is the Moon so high (or so Low)? ? Amateur Astronomers Association of New
... Home Articles Why is the Moon so high (or so Low)? ... Clear Sky Chart . This Month's Sky . ... Beyond New York City . ... Why is the Moon so high (or so Low)? ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . Observing Resources for Amateur Astronomers - Part 2: Intermediate Observers . ... A History of the First Forty Years of the Amateur Astronomers Association . ... 2016 Amateur Astronomers Association of New York Designed by Press Customizr Powered by . ...
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Ссылки http://www.aaa.org/articles/why-is-the-moon-so-high-or-so-low/ -- 111.9 Кб -- 10.04.2016
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103. COSMIC RAY Observation
Cosmic Ray laboratory of . ... Neutron Monitor (Cosmic Ray Observations) . is situated in Irkutsk (Russia) . ... Height - location above sea level . ... Height: . ... For recording the CR (Cosmic Rays) neutron component at Irkutsk, . neutron monitor NM-64 is used, which is an installation with 18 two-meter proportional counters filled with BF 3 (boron trifluoride gas) in which the B 10 90 per cent of the total boron. ... The neutron monitor is located at 475m above sea level. ...
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Ссылки http://cgm.iszf.irk.ru/irkt/about.htm -- 3.9 Кб -- 10.01.2005
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104. http://ikfia.ysn.ru/english/Aurora.html
Aurora and Nightglow Laboratory . Head Dr. Valery Alexeyev . Phone: +7(4112) 39-04-60 . Fax: +7(4112) 39-04-50 . ... Dr. Peter Ammosov . Dr. Galina Gavrileva . Dr. Igor Ievenko . ... Dr. Semen Nikolashkin . Electronics engineer Nikolay Alexeyev . Post-graduate Igor Koltovskoy . Post-graduate Stanislav Parnikov . Post-graduate Galina Timofeeva . Post-graduate Semen Titov . ...
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Ссылки http://ikfia.ysn.ru/english/Aurora.html -- 3.2 Кб -- 21.11.2013
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105. http://site2010.sai.msu.ru/static/doc/GHerriot_site2010.ppt.pdf
Using Site testing data for Adaptive Optics simulations Kislovodsk, October 2010 1Glen Herriot, 1David Andersen, 1Jean-Pierre VИran, 2Brent Ellerbroek, 2Luc Gilles, 2Lianqi Wang 1National Research Council Canada Herzberg Institute of Astrophysics 2TMT Project Office, Pasadena TMT.AOS.PRE.10.074.REL01 1 Outline TMT / NFIRAOS Site Testing Parameters and their value for Adaptive Optics Simulations ... TMT.AOS.PRE.10.074.REL01 9 What is the interest of Adaptive Optics in r 0 Seeing ? ...
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Ссылки http://site2010.sai.msu.ru/static/doc/GHerriot_site2010.ppt.pdf -- 1942.1 Кб -- 18.10.2010
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106. http://sn.sai.msu.ru/~sil/preprints/aspb121.pdf
... Properties of Stellar Populations in Isolated Lenticular Galaxies I. Yu. ... The resulting average ages of the stellar population in bulges and discs fill an entire range of possible values from 1.5 to 15 Gyr which indicates the absence in the isolated lenticular galaxies, unlike in the members of groups and clusters, of a certain epoch when the structural components are formed: they could have been formed at a redshift of z > 2 as well as only several billion years ago. ... 69 NGC 2350 No. ...
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Ссылки http://sn.sai.msu.ru/~sil/preprints/aspb121.pdf -- 1591.8 Кб -- 11.07.2015
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