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201. http://kcor.sai.msu.ru/arXiv1002.2360.pdf
... 000, 1­12 (2009) Printed 11 February 2010 A (MN L TEX style file v2.2) Analytical approximations of K -corrections in optical and near-infrared bands I1gor V. Chilingarian1 2 ,2,3 , Anne-Laure Melchior 1,4 and Ivan Yu. ... Received 2010 February 01; in original form 2009 August 14 ABSTRACT To compare photometric properties of galaxies at different redshifts, the fluxes need to be corrected for the changes of effective rest-frame wavelengths of filter bandpasses, called K -corrections. ... Table 1. ...
[ Текст ]  Ссылки http://kcor.sai.msu.ru/arXiv1002.2360.pdf -- 1631.3 Кб -- 12.02.2010
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202. Молодежное Астрономическое Общество
... Появилось Одесское Молодежное Астрономическое Общество (Одесса).. ... Одесское Молодежное Астрономическое Общество (Одесса),(далее просто МАО) ? ... Для помощи этим людям и создано МАО. ... Ждем в гости: Одесса-14, парк им. Шевченко, Одесская Астрономическая Обсерватория...лучше заранее позвоните:8-0482(код Одессы), 69-24-30 (Юра), 66-45-70 (Саша), 45-13-32(Витя), 715-49-15(Максим), 25-03-56 (Одесская Астрономическая Обсерватория). наши e-mails: maoclub@ukr.net и mao_webmaster@ukr.net . ...
[ Сохраненная копия ]  Ссылки http://www.maocity.narod.ru/ -- 13.8 Кб -- 09.04.2016
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203. http://site2010.sai.msu.ru/static/doc/VOrlov_site2010.pdf
Dynamic Shack-Hartmann System RAPID V. G. Orlov, V. V. Voitsekhovich Instituto de AstronomМa, UNAM, MИxico CONACYT project E9507-1020P UNAM PAPIIT IN104910 Telescopes OAN OAN- SPM 2.1m telescope 1.5m telescope 0.84m telescope 2.1m telescope OAN-Tonanzintla 1m telescope Astronomical site SPM Observing statistics 1982-2002 (Tapia+ 2007 ) Photometric nights : 64.1% Spectroscopic ... Rapid - Dynamic Shack-Hartmann All modern telescopes demand installation of adaptive system. ...
[ Текст ]  Ссылки http://site2010.sai.msu.ru/static/doc/VOrlov_site2010.pdf -- 1652.8 Кб -- 18.10.2010
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204. http://sn.sai.msu.ru/~sil/preprints/postbr1.pdf
... The circumnuclear GASEOUS disks are often decoupled from the circumnuclear stellar disks and are even stronger inclined to the outer disk planes; in fact, we have found a considerable `population' of inner polar rings. Inner gas polar rings are found as in spiral galaxies with the massive outer gas disks co-planar to the main symmetry planes (e.g. NGC 2841, Sil'chenko et al. 1997, and NGC 7217, Sil'chenko & Afanasiev 2000) as well in many lenticular galaxies (Fig. ...
[ Текст ]  Ссылки http://sn.sai.msu.ru/~sil/preprints/postbr1.pdf -- 76.8 Кб -- 01.12.2004
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205. 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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206. What is Redshift? (2dF QSO Redshift Survey - 2QZ)
... Under certain conditions, like those in the nucleus of a QSO, all atoms can be made to emit light at particular wavelengths. ... If that source is approaching the observer, the wave is squashed up onto itself making the wavelength shorter. ... This is redshift. ... You can see how the section of the QSO spectrum which we observe changes with redshift. ... We then see how far we had to slide the observed spectrum along the scale to make it match and that is the objects redshift. ... The 2QZ team . ...
[ Сохраненная копия ]  Ссылки http://www.2dfquasar.org/restframe.html -- 10.2 Кб -- 07.05.2008
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207. GLOOBUS-M diagnostics
The low aspect ratio, or spherical tokamak Globus-M [1] has recently been built in a support of international spherical tokamak plasma investigation program. ... The survey to determine the work scope in diagnostic design for Globus-M is given in the paper. ... The next one is an advanced diagnostic set intended to supply the data on basic plasma parameters: electron temperature and density profiles, ion temperature, plasma composition, radiation profile, Zeffective. ... Magnetic Diagnostics. ...
[ Сохраненная копия ]  Ссылки http://www.ioffe.rssi.ru/HTPPL/GLOBUS-M/diagnostics.html -- 20.0 Кб -- 17.10.2012
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208. http://xmm.vilspa.esa.es/sas/5.4.1/doc/saslib/rfc1321.txt
... April 1992 The MD5 Message-Digest Algorithm Status of this Memo This memo provides information for the Internet community. ... combination): -sstring - digests string -t - runs time trial -x - runs test script filename - digests file (none) - digests standard input */ int main (argc, argv) int argc; Rivest [Page 17] RFC 1321 MD5 Message-Digest Algorithm April 1992 char *argv[]; { int i; if (argc 1) for (i = 1; i argc; i++) if (argv[i][0] == '-' argv[i][1] == 's') MDString (argv ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/5.4.1/doc/saslib/rfc1321.txt -- 35.4 Кб -- 06.04.1993
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209. http://cgm.iszf.irk.ru/irkt/info.htm
... GCR and SCR are primary cosmic rays. 10-15 years after the discovery of cosmic radiation (1919) there emerged two main avenues of investigation in the physics of cosmic rays (CR): 1) nuclear - elucidation of the origin of elementary particles and nuclear interactions; and 2) astrophysical (space physics) - solution of the problem related to the origin and variations (changes in intensity) of CR. ... Besides, the CR flux in interplanetary space is, strictly speaking, not isotropic. ...
[ Сохраненная копия ]  Ссылки http://cgm.iszf.irk.ru/irkt/info.htm -- 6.1 Кб -- 28.11.2002
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210. Kinematics of galaxies: supplement
We present a catalogue of galaxies for which spatially resolved data on their internal kinematics have been published; there is no apriori restriction regarding their morphological type. The catalogue lists the references to the articles where the data are published, as well as a coded description of these data: observed emission (E) or absorption (A) data, optical (O) or radio (R) data, velocity (V) or velocity dispersion (D), radial profile (1) or 2D field (2). ...
[ Сохраненная копия ]  Ссылки http://neptun.sai.msu.su/~zasov/comcat.htm -- 2.4 Кб -- 15.01.1999
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