... ОМНОЕИ К ?Д Й КП НЙП ОК Йб а кг з гКжй ПН Н О НК И И НИ ? ... Й И Й Й К Й И Й Й Й Й О И К И К S > 10 И И И Д И И Й ЦЙ К ЕК И И КН П ОН И иид ЛЛлллК кКвж гК йЛ ж а Л б Д К НЕИ ПО П ПНИ зК ибК Ъ С СК Ъ СК И Д СЪЫЬ Д И К? К К К Ъ Н П ЕИ Д ги зд гиз ЕК И И ЮФ г Ыйжк н и Ьл вин бЕ И К И К К Д И Й ви Сб Е З y = A + B xИ З y = A + B x + C x2 И З y = A + B x + C ex И З y = A + B x + C e-x И y = log10(S )И x = log10( )И S И ДКК ЕИ И ДТнЕ Д Д ЕИ Й бТнЕ Н К ?К Й И Й Й Д КИ Й К Й Й Й Ъ С СК И ЕК ? ...

... Average effective wavelengths and band widths for various sp ectra Lyrae spectrum f flat k е 1014 Hz 5386 ± 18 4.66 ± 0.04 5714 ± 12 4.1 6234.5 ± 0.5 1.03 5372 ± 18 4.69 ± 0.04 eff 2 Optical Filter ID 1 2 3 4 a Fo c -6 10 erg/cm2 s 12.55 ± 0.10 11.04 ± 0.01 2.77 ± 0.004 12.63 ± 0.10 fo d 6 10 photons/cm2 s 3.40 ± 0.02 3.18 ± 0.004 0.87 ± 0.002 3.42 ± 0.02 Power-law eff f 2 е 5746 ± 317 6197 ± 253 6305 ± 31 5736 ± 316 spectra pl k 1014 Hz 3.70 ± 0.26 3.14 ± 0.16 0.88 ± 0.01 3.70 ± 0.27 Table 1. ...

Geomagnetism and Aeronomy, Vol. 45, No. 6, 2005, pp. 681­719. Translated from Geomagnetizm i Aeronomiya, Vol. 45, No. 6, 2005, pp. 723­763. Original Russian Text Copyright © 2005 by Yu. Yermolaev, Zelenyi, Zastenker, Petrukovich, M. Yermolaev, Nikolaeva, Panasyuk, Kuznetsov, Myagkova, Murav'eva, Yushkov, Veselovsky, Dmitriev, Zhukov, Yakovchouk, Kuznetsov, Chertok, Ishkov, Belov, Eroshenko, Yanke, Gaidash, Kanonidi, Kuzin, Zhitnik, Ignat'ev, Slemzin, Sukhodrev, Shestov, M. Eselevich, V. Eselevich, Rudenko,

R And S5/4.5e. S And SN (NGC 224). W And S7.5/1-e. X And S5/7-e. Z And The light curve is characterized by outbursts up to 4m with intervals of 10 - 20 years. In the intervals cyclic variations are observed with the mean period of 632d and variations with cycles of several days and Delta(m) ~ 0.1m - 0.5m. The spectrum is symbiotic, with features of a late M giant, narrow low-excitation emission lines (Bleq) and forbidden lines characteristic of highly excited nebulae. RR And S6/3.5e. RT And Min II 8.88; DI

. Computer Ephemeris for 2014 from DE200/LE200. Mean places of fundamental stars at J2014.5 # name m Sp paralax alpha dif mu(al) delta dif mu(dl) " h m s s s o ' " " " 902 Psc omega 4.01 F5 0.012 3.437 3.085 0.0103 65636.77 19.93 -1.15 903 Tuc epsilon 4.50 B9 0.000 39.621 3.084 0.0077 -652947.46 20.02 -0.24 904 Oct theta 4.78 K0 0.011 219.259 3.016 -0.0188 -765908.52 19.86 -1.77 1630 Psc 30 4.41 M3 0.043 242.249 3.077 0.0034 -55600.70 20.00 -0.41 905 Cet 2 4.55 A0 0.004 428.899 3.070 0.0018 -171519.15 20.03

Supernova 2000ew in NGC 3810 . This page is devoted to information on Supernova 2000ew in NGC 3810 Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . Information on the original web pages for many of these images can be found on the Supernova links web page. Another discovery by Puckett Observatory . This one in a fairly bright nearby galaxy. ... JM Llapasset image . ... vsnet-alert 5412 ] SN 2000ew in NGC 3810 . ...