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121. http://sun.sai.msu.ru/texts/somov-1-10Lect.pdf
Introduction to PLASMA ASTROPHYSICS (Selected 10 lectures) Boris V. Somov Astronomical Institute and Faculty of Physics Moscow State University Pushino-na-Oke, 2008 Contents Ab out These Lectures 1 Particles and Fields: Exact Self-Consistent Description 1.1 Liouville's theorem . . . . . . . . . . . . . . . . . . . 1.1.1 Continuity in phase space . . . . . . . . . 1.1.2 The character of particle interactions 1.1.3 The Lorentz force, gravity . . . . . . . . . 1.1.4 Collisional friction . . . . . . . . . . . .
[ Текст ]  Ссылки http://sun.sai.msu.ru/texts/somov-1-10Lect.pdf -- 1179.0 Кб -- 18.03.2014
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122. The VSM: About this site
... Official logo of the VSM - Who and Where? What's here? ... This site's goal - The Virtual Space Museum is currently located at the Computing Center of Russian Academy of Science ( CC RAS ). ... Here you'll find mainly VRML models of Russian spacecraft and launch facilities. ... The VSM's goal is to let you see all the Russian cosmonautics rather than to provide you with encyclopaedic information. If you need figures and descriptions, try sites listed in the Links section. ...
[ Сохраненная копия ]  Ссылки http://www.vsm.host.ru/about.htm -- 3.0 Кб -- 24.05.1999
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123. http://www.inasan.rssi.ru/~kurbatov/Kurbatov--arXiv-1012.1216.pdf
The Influence of the Decay of OB Associations on the Evolution of Dwarf Galaxies E. P. Kurbatov arXiv:1012.1216v1 [astro-ph.GA] 6 Dec 2010 Institute of astronomy, Russian Academy of Sciences 48 Pyatnitskaya st., Moscow, Russian Federation, 119017 kurbatov@inasan.ru Abstract It is commonly b elieved that most of the stars b orn in asso ciations decaying with characteristic velo cities of stars 10 km/s. For dwarf galaxies the decay can lead to ejection of stars from the galaxy. ... Galactic dynamics. ...
[ Текст ]  Ссылки http://www.inasan.rssi.ru/~kurbatov/Kurbatov--arXiv-1012.1216.pdf -- 232.6 Кб -- 06.09.2012
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124. 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. ...
[ Текст ]  Ссылки http://www.2dfquasar.org/Papers/2002MNRAS.337..275C.pdf -- 831.9 Кб -- 04.03.2004
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125. http://www.sai.msu.su/gcvs/digit/mdv/MDV1.pdf
... 8 s h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h h GSC / USNO-A2.0 A A A G A G A A A G A G A A G A A A G A G A A A A A G A A A A G G A A A A G A A A G A A A A A A A A A G G A G A A G ... -10884039 975-09978626 975-09980031 900-10928663 900-10939727 975-09994108 900-10948278 975-10003602 900-10962191 975-10012892 t ype LB RRA B RRA B SR: EB SRB EW RRA B EW LB RRA B LB RRA B SRB EW EW ... Variable in NSVS data. ...
[ Текст ]  Ссылки http://www.sai.msu.su/gcvs/digit/mdv/MDV1.pdf -- 459.5 Кб -- 06.12.2011
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