... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. December 18, 1999 . Irregular Galaxy Sextans A . ... Their newly formed, bright, blue star clusters found along beautiful, symmetric spiral arms are guaranteed to attract attention. But small irregular galaxies form stars too , like this lovely, gumdrop-shaped galaxy, Sextans A . ... About APOD > . ...

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• APOD: December 27, 1995 - Nova Cygni 1992

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• GCalendar: Декабря 1630
• GCalendar: Декабря 1631
• GCalendar: Декабря 1632

... 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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• http://sn.sai.msu.ru/~sil/preprints/my_an.pdf
• http://sn.sai.msu.ru/~sil/preprints/ic719.pdf
• http://sn.sai.msu.ru/~sil/preprints/ilyina_sil.pdf

... Supercomputing Technologies in Science, Education and Industry Almanac Series . ... Keldysh Institute of Applied Mathematics of RAS . DRIVER: 3D numerical modelling of high energy density plasma physics . ... AREA: Plasma Physics . ... IMPACT: The expected results of numerical experiments will help to explain the observed statistical characteristics of molecular hydrogen clouds in external galaxies. ... Research Computing Center (RCC) of Lomonosov Moscow State University . ...

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• APPLICATIONS: Astronomy | Moscow University Supercomputing Center

... Bohm limit DB=vrg/3: Emax Emax ush 0.3 Ze B Rsh c 1014(B/Bism) Z eV B Hillas criterion ! ... Voelk 2000; Kang Jones 2006) - Bohm diffusion in amplified magnetic field B2/8 = 0.035 u2/2 ( Voelk et al. 2005 empirical; Bell 2004 , Zirakashvili VP 2008 theoretical) - account for Alfvenic drift w = u + Va upstream and downstream - relative SNR rates: SN Ia : IIP : Ib/c : IIb = 0.32 : 0.44 : 0.22 : 0.02 Chevalier 2004 , Leaman 2008, Smart et al 2004, Berezinsky et al 2006 Das et al. ...