... 1997-2000 ) - (0-117) , .. 2001 . ... a. ppa . ... a (a paa), pa . ... 1999 "" - . ... 1 31 1997 , , 1 1998 , . ... p a pa a apa pa; ! ... a, ap aa a a ppa paa apa a p p p p a paa P. - . ... 5 2000/2001 317 9.00-10.35 12.40-14.15 .. ... p pp apap p p pa. 2. paa ppa ppa Ї Ppa ppa ap pa a p pap. Ї paa pa ppa pa ap ppa paa paa pap. Ї pp pa ppa AREN (pa pp a, R-apa, p p apa). Ї a pa a pa p p (a pa ppa, ). ... 100 80 60 40 20 0 1997 1998 1999 2000 38 100 80 60 40 20 0 1997 1998 1999 2000 , 250 , . ...
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... In the light curve depicting their observations, definite trends are noted, here is a "thumb-nail" analysis of the the magnitude estimations of the bright SN (1989B) in the galaxy NGC 3627 (M66). ... 10 (IAUC # 4742) 2/25 13.3 16 j 2/27 13.5(*) 18 lc 2/28 13.8 19 p 3/1 13.2 20 w 3/2 13.5 21 a 3/4 13.8 23 p 3/6 13.3 25 c 3/7 13.3 26 c 3/8 14.1 27 m 3/8 13.3 27 r 3/9 13.4 28 c 3/9 14.1 28 m 3/10 13.6 29 j 3/10 14.0 29 a 3/11 13.6 30 c 3/11 13.5 30 r 3/11 13.7 30 s 3/13 [13.69 CCD Mag.] ...
... sought for such use through Elsevier's permissions site at: http://www.elsevier.com/locate/permissionusematerial ARTICLE IN PRESS JOURNAL OF SOUND AND VIBRATION Journal of Sound and Vibration 298 (2006) 471 - 474 www.elsevier.com/locate/jsvi Short Communication Wolfhard Kliema, Alexei A. Mailybaevb,Г, Christian Pommer a copy Conditions revisited for asymptotic stability of pervasive damped linear ... In the case of an indefinite damping matrix, system (1) may be stable or unstable. ...
... Structural Analysis of Disk Galaxies of the NGC 524 Group M. A. Il'ina and O. K. Sil'chenko * Sternberg Astronomical Institute, Lomonosov Moscow State University, Moscow, Russia Received February 24, 2012; in final form, March 2, 2012 Abstract--Members of the NGC 524 group of galaxies are studied using data obtained on the 6m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences, with the SCORPIO reducer in an imaging mode. ... NGC 502. ... NGC 524. ... Rev. Astron. ...
... 000, 1ґ13 (2010) Printed 21 September 2011 A (MN L TEX style file v2.2) A universal ultraviolet-optical colourґcolourґmagnitude relation of galaxies I1gor V. Chilingarian1,2, and Ivan Yu. ... Received 2011 Sep 15; in original form 2011 Feb 6 ABSTRACT The bimodal galaxy distribution in the optical colourґmagnitude diagram (CMD) comprises a narrow "red sequence" populated mostly by early-type galaxies and a broad "blue cloud" dominated by star-forming systems. ...