... Глава 12. ... Каждая из двух окружностей касается обеих сторон данного прямого угла. Найдите отношение радиусов окружностей, если известно, что одна из них проходит через центр другой. ... Докажите, что радиусы окружностей, описанных около треугольников ACM , BDK , ACK , BDM , связаны соотношением R ACM ћ R BDK = R ACK ћ R BDM . ... Найдите радиус окружности, проходящей через точки касания этих окружностей. ... Найдите радиус вписанной окружности, если известны радиусы этих окружностей. ...
Searching for an Optimal Strategy to Intensify Observations of the Southern ICRF sources in the framework of the regular IVS observing programs ? ... We found that adding more observations of southern sources to the standard schedule causes a slight degradation of some geodetic products and a slight improvement of others, depending on the number of added southern sources. ... As a consequence, the number of observations of the southern sources is very small. ...
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Ссылки http://www.gao.spb.ru/english/personal/malkin/publ/zm13o.pdf -- 136.2 Кб -- 08.11.2013 Похожие документы
... Our most pressing need is to maintain the number of visitors coming to see our shows and displays. ... Armagh Planetarium Business Plan 2009 / 2010 Review of Key Objectives for the 2008 2009 Financial year Armagh Planetarium 's key performance indicators for the 2008 2009 Financial year were: KEY PERFORMANCE INDICATORS KPI Visitor numbers Outreach numbers Virtual Planetarium visitors (since September) Internet hits per day TSN numbers 1 Admissions income ...
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Ссылки http://www.armaghplanet.com/pdf/Administration/business%20plan_2009_2010.pdf -- 438.7 Кб -- 20.09.2011 Похожие документы
... Построение интерактивной графической системы обработки (69) . ... Подобные системы обработки данных зачастую бывают довольно громоздкими. ... Начиная с 1994 года (Верходанов и др., 1994), система обработки радиоастрономических данных FADPS использует FITS Binary Table-подобный формат (Harten et al., ... Чистка и редукция наблюдений осуществлялась с помощью пакета fgr (Верходанов, 1995a) в стандартной системе обработки континуальных данных на РАТАН-600 FADPS (Verkhodanov et al., ... Спектры объектов....
... Астрономические мероприятия (Модераторы: mak , DF ) > . УАФ 2011 - отчет . ... Мероприятия . Отчеты о наблюдениях . ... Астрономический кружок гимназии ?59 г. Киева . ... Благодарностей: 45 . ... Ответ #20 : 10 Май 2011, 20:14:56 ? ... Благодарностей: 1001 . ... Цитата: DF от 10 Май 2011, 21:17:33 сохраните как файл с раширением air, а потом запустите приложение. ... Наверное, лучше все же позже, но рассказать о том, как все проходило. 01.jpg (273.66 КБ, 550x827 - просмотрено 125 раз.) ...
... We quote the 2 per degree of freedom of the best fitting line and the significance of the fit for each regression in Table 4. ... 43 Table 2--Continued Exp eriment Ref. eff m in max T obs ± obs eff a c Publication Date (yrs) 2001.2 2001.2 2001.2 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 ...
... It is found that single crystals of different phases of the family can be prepared if the electrocrystallization medium is represented by the mixture of 1,2,4-trichlorobenzene (or 1,3-dibromobenzene), 96% ethanol and different solvents (G), only the latter being included into the composition of the resulting salts as neutral guest molecules (G ј benzonitrile, fluorobenzene, chlorobenzene, 1,2-dichlorobenzene, bromobenzene, nitrobenzene). ... The resulting solvent compositions are listed in Table 1. ...
. Bright Supernovae - 2011 . This data comes from IAU Circulars and occasionally more data will be provided on IAU 's Astronomical Headlines page. An archive of the 2011 updates to this page is available. This is a partial list of the SN discovered in 2011. Since 2011 is still ongoing, please look at the main page for the latest data. Note that Extra galactic Novae have been moved to a special Extra galactic novae page . For more information, you can look at the following Supernova Catalogs: . IAU List of
CMi CMi CMi Cam Cam Cas Cas Cas Cas Cas Cas Cep Cep Cep Cep Cep Cep Cep Cep Cnc Cnc CrA Crv Cyg Cyg Cyg Cyg Cyg Cyg Cyg Cyg Cat MINK NGC ABELL ABELL ABELL ABELL ABELL ABELL ABELL ABELL IC MINK NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC SH2 NGC NGC ABELL IC IC NGC ABELL IC ABELL ABELL ABELL IC NGC ABELL ABELL ABELL ABELL IC IC ABELL ABELL IC MINK NGC NGC NGC NGC ABELL ABELL IC NGC ABELL ABELL ABELL HENIZ ...
... 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. ...
... Рейтинг страниц в теме: . ... Оценено и сдано в архив! . ... Gazinur Galazutdinov home page . ... Sergei Shugarov Home Page . ... Vladimir Il'in's home page . ... Natalia Sotnikova's Home Page . ... Alexander V. Krivov's Home Page . ... Equinox - праздник осеннего равноденствия в ГАИШе . ... N. Pavlyuk home page . ... Renat Zagretdinov home page . ... Alexei Moiseev Home Page . ... Valery V. Dikarev's Home Page . ... НАЗАД, В СПИСОК КАТЕГОРИЙ (титульная страница AstroTop-100) . ...
R And SiO maser. S And SN (NGC 224). W And SiO maser. Z And Outbursts, average cycle 8400d. Porb = 758.8d, it reveals Z And itself in photometry during the low state. A quasi-period, P1, Z And about 656d is present during the outbursts. The beat period Z And between Porb and P1, about 5500d, is also found in the Z And photometric data. RS And H2O maser. RT And Min II = 9.28. P varies, current elements are given. RU And P varies strongly. RX And Porb = 0.209893d. RY And OH, H2O maser. SS And P2 = 650d, P3 =
\documentstyle[twoside]{article} \input ibvs2.sty \begin{document} \IBVShead{4870}{31 March 2000} \IBVStitle{The 75th Name-List of Variable Stars} \IBVSauth{Kazarovets, E.V.$^1$; Samus, N.N.$^1$; Durlevich, O.V.$^2$} \IBVSinst{Institute of Astronomy, Russian Academy of Sciences, 48, Pyatnitskaya Str., Moscow 109017, Russia\\ \indent [samus@sai.msu.ru, elena\_k@sai.msu.ru]} \IBVSinst{Sternberg Astronomical Institute, University of Moscow, 13, University Ave., Moscow 119899, Russia \\ \indent
RT And * CB EA RS 8.97 0.41 0.31 V 0.6289 v 170 000 170 000 F8V+K1 a 231110.1 +530133 SY And SA * EA 10.70 1.50 V 34.9085 060 027 A0+K1 001316.4 +434241 TT And * SA EA 11.50 1.50 0.10 V 2.7651 v 140 000 A+G7IV 231322.9 +460851 TW And * SA EA 8.98 2.06 0.15 V 4.1228 v 130 020 F0V+K0 000318.2 +325045 UU And SA EA 11.20 3.00 0.20 V 1.4863 v 170 000 A8IV/V 004345.1 +305620 WW And * SA EA 10.92 0.67 0.16 V 23.2852 050 000 000 A0:+G5-K0III 234453.5 +454112 WX And SA * EA 12.10 1.70 V 3.0011 d 120 030 F5IV