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201. http://www.stecf.org/conferences/adass/adassVII/reprints/oknyanskijv.ps.gz
... Methodology of Time Delay Change Determination for Uneven Data Sets V.L.Oknyanskij Sternberg Astronomical Ins., ... It was found in this way that the radio variations (5 MHz) followed the optical ones, but that the time delay was a linear function of time with the mean value being about 2370 days and with the rate of increase V # 110 days/year. ... Time Delay Change Determination for Uneven Data Sets 491 Figure 2. p(V) is probability to get some value V # # V if the actual V a = 0 days/year. ...
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Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/oknyanskijv.ps.gz -- 103.6 Кб -- 12.06.2006
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202. http://www.princetonastronomy.org/newsletters/07_2009sidereal.pdf
... Our first meeting of the year will be on Tuesday, September 8th. ... next page) Page 2 Amateur Astronomers Association of Princeton Newsletter Revenue and Expenses General Operations Actual Ordinary Income /Expense Income Contribution Income Member Dues Outreach Contributions Sale of Equipment Sales of AAAP Astro Items StarQuest Attendance Total Income Expense Speaker Honorarium Astronomy Calendars Books and Publications Business License Fees Contribution Expense Dues and ...
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Ссылки http://www.princetonastronomy.org/newsletters/07_2009sidereal.pdf -- 990.6 Кб -- 30.07.2009
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203. http://sn.sai.msu.ru/~sil/preprints/486-0027.pdf
... 486 Enrichetta Iodice and Enrico Maria Corsini, eds. c 2014 Astronomical Society of the Pacific Inner Polar Gaseous Disks: Incidence, Ages, and Possible Origin O. K. Sil'chenko1 and A. V. Moiseev2 Sternberg Astronomical Institute, Lomonosov Moscow State University, Moscow, Russia Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnii Arkhyz, Russia Abstract. ... Further Bettoni et al. (1990) have claimed inner polar gaseous disk in the Southern ringed lenticular galaxy NGC 2217. ...
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Ссылки http://sn.sai.msu.ru/~sil/preprints/486-0027.pdf -- 174.7 Кб -- 12.07.2015
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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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205. http://www.armaghplanet.com/pdf/Administration/AnnualReportAccounts_2010-2011.pdf
The Armagh Observatory and Planetarium Annual Report and Accounts for 2010/2011 Year Ended 31 March 2011 © Armagh Observatory and Planetarium Copyright 2011 You may re-use this document/publication (not including logos) free of charge in any format or medium, under the terms of the Open Government Licence. To view this licence, please visit http://www.nationalarchives.gov.uk/doc/open-government-licence. For further details about the re-use of Armagh Observatory and Planetarium information please write to
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Ссылки http://www.armaghplanet.com/pdf/Administration/AnnualReportAccounts_2010-2011.pdf -- 769.1 Кб -- 10.11.2011
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