... Любительская фотография (Модераторы: eone , veifert ) > . ... Оффлайн . Сообщений: 5658 . Благодарностей: 113 . Ответ #20 : 09 Октябрь 2011, 12:57:15 ? ... Записан . ... Цитата: Серега от 09 Октябрь 2011, 13:05:29 шо это за тетка? и вообще о чем речь? . ... Цитата: Vagabond от 09 Октябрь 2011, 13:09:39 а что это за бэтмен в ответе ?15?? . ... Цитата: Серега от 09 Октябрь 2011, 15:27:59 а то тоже недавно в киеве было, правда без пожара, не угадаете кто - значит все запущено : . ...

The Official Publication of the Amateur Astronomers Association of Princeton Director John Miller (609) 252-1223 jmiller@princetonastronomy.org Assistant Director John Church (609) 799-0723 j.church@mindspring.com Treasurer Program Chairman Michael Mitrano Ludy D'Angelo 609-737-6518 (609) 882-9336 michael .mitrano@worldnet.att.net ldangelo106@comcast.net Secretary Editors Ron Mittelstaedt Bryan Hubbard and Ira Polans (609) 771-6981 (732)-469-7698 and (609)448-8644 ...

... This is commonly referred to as CPM (cost per thousand impressions).We pay you a percentage of revenues for the ads that you and your friends view with Harry, based on current CPM rates.You will get 75% of total revenue generated from your viewing.. ... REMEMBER: for every one hour the program on Your screen You'll get paid $0.50. And when You recommend those program to Your friends, reffering to Your personal ID, You'll get paid $0.10 for every hour the program open on Your's friends computer. ...

... 33, No. 1, pp. 62­71. i Formation of Power-Law Electron Spectra in Collapsing Magnetic Traps S. A. Bogachev 1 1* and B. V. Somov 2** Lebedev Institute of Physics, Russian Academy of Sciences, Leninski i pr. ... It is shown that if the electrons injected into the trap have a power-law spectrum, then their spectrum remains a power-law one with the same slope throughout the acceleration process for both the Fermi and betatron acceleration mechanisms. ... They do not coincide at energies below 20 keV. ...

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... Cependant tout portait єђ croire au succє¦s, puisque le moule avait absorbєµ la masse entiє¦re du mєµtal liquєµfiєµ dans les fours. ... Combien de temps, dє¦s lors, la monstrueuse Columbiad, couronnєµe de ses tourbillons de vapeurs, et dєµfendue par sa chaleur intense, allait-elle se dєµrober aux regards de ses admirateurs? ... L'impatience des membres du Gun-Club fut mise pendant ce laps de temps єђ une rude єµpreuve. ... Les jours s'єµcoulє¦rent, les semaines s'ajoutє¦rent l'une єђ l'autre. ...

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Russian . ... Very Early Universe: inflation, generation of primordial perturbations, preheating . Very Early Universe: inflation, generation of initial perturbations, preheating . Cosmic Microwave Background Radiation: anisotropy and polarization . ... Dark Energy and Dark Matter models . High Energy Astrophysics: accretion discs, cosmic rays, gamma-ray bursts . ... Astrophysics of black holes and wormholes . ...

... 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. ...

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 . . . . . . . . . . . .