Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...

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• Structure of the Galaxy
• Gamma-Ray Bursts
• Calculation of Binary Neutron Star Coalescence Rates

Электронная библиотека Попечительского совета . ... Appenzeller I. (ed.), Habing H.J. (ed.), L?na P. (ed.) - Evolution of Galaxies Astronomical Observations . ... Название: Evolution of Galaxies Astronomical Observations . Авторы: Appenzeller I. (ed.), Habing H.J. (ed.), L?na P. (ed.) . ... Bias mechanisms for galaxy formation 72 . ... Chemical evolution 172 . ... Color evolution 168 . ... Galactic chem. evolution 151 . ... Электронная библиотека попечительского совета мехмата МГУ , 2004-2016 . ...

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• Padmanabhan T. - Structure Formation in the Universe :: Электронная библиотека
• Keel W.C. - The Road to Galaxy Formation :: Электронная библиотека
• Padmanabhan T. - Theoretical astrophysics, vol. 3 :: Электронная библиотека

... Moscow, Russia . ... March-October 2000 . ... Gusev A.S. Multicolor CCD Photometry of Six Lenticular and Spiral Galaxies. ... Gusev A.S., Park M.-G. Structure and stellar population of ringed barred galaxy NGC 2336 // Astronomy and Astrophysics, 2003, V.410, P.117-129. ... Gusev A.S. Photometric Properties of Bars in Galaxies // Astronomy Reports, 2000, V.44, N9, P.579-591. ... Gusev A.S. BVRI CCD Photometry of Pecular Galaxies NGC 5605 and NGC 5665 // Astronomy Reports, 2000, V.44, N9, P.569-578. ...

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• Maidanak Lab page
• Yuri Nicolaevich Efremov - My Home Page

... Program of the Course of Radio Astronomy . Moscow State University , Physics Department , Astronomy Division , 4 th year, 60 hours in total) . ... Molecular maser emission. ... The emission of the interstellar neutral hydrogen. ... Pacholczyk, A. G. Radio Astrophysics, W. H. Freeman & Co., ... Frontiers of Astrophysics, Avrett, E. H., ed., Harvard University Press, Cambridge, Mass., ... Kaplan, S. A., Pikelner, S. B. The Interstellar Medium, Harvard University Press, Cambridge, Mass., ...

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• http://comet.sai.msu.ru/~dmbiz/abst/dd-a

... Galaxy Collisions: Simulation vs Observations . ... 14.05.2013 . ... Explanation: What happens when two galaxies collide? ... Since galaxies are mostly empty space, no internal stars are likely to themselves collide . ... Pictured above is a computer simulation of two large spiral galaxies colliding , interspersed with real still images taken by the Hubble Space Telescope . ... May 2013 . ... Publications with keywords: colliding galaxies . Publications with words: colliding galaxies . ...

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• Астронет > Galaxy Collisions: Simulation vs Observations
• Astronet > Sky Map, professional edition
• Leo A: Nearby Dwarf Irregular Galaxy

... 2013 May 14 . Galaxy Collisions: Simulation vs Observations . Images Credit: NASA , ESA ; Visualization: Frank Summers ( STScI ); Simulation: Chris Mihos ( CWRU ) Lars Hernquist ( Harvard ). Explanation: What happens when two galaxies collide? Although it may take over a billion years, such titanic clashes are quite common. ... Pictured above is a computer simulation of two large spiral galaxies colliding , interspersed with real still images taken by the Hubble Space Telescope . ...

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• Zen: sncat design
• APOD: 2004 November 10 - Leo A: Nearby Dwarf Irregular Galaxy
• APOD: 2007 May 16 - Dark Matter Ring Modeled around Galaxy Cluster CL0024 17

Выберите категорию обращения: Общие вопросы Отчеты Рейтинги Диссертационные советы Конкурсы Ввод данных Структура организаций Пользователи Проблемы с регистрацией\входом в систему . ... Войти в систему . ... Fridman A.M. , Afanasiev V.L. , Dodonov S.N., Khoruzhii O.V. , Moiseev A.V. , Sil?chenko O.K. , Zasov A.V. в журнале Astronomy and Astrophysics , издательство Springer Verlag (Germany) , том 430, ? ...

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• Burenkov A.N. - сотрудник | ИСТИНА - Интеллектуальная Система Тематического
• Sakhibov F.Kh - сотрудник | ИСТИНА - Интеллектуальная Система Тематического
• Turolla R. - сотрудник | ИСТИНА - Интеллектуальная Система Тематического

Teaching courses . for student of the Department of Astrophysics and Stellar Astronomy . ... Geophysics and physics of the planets (Kurt, Panteleev) . ... Close Binary Stars . ... Solar Physics . ... This is introductory course for students of the third year of education which are familiar with elementary astronomy and general physics. ... The one-year course includes theory of radiation transfer, theory of internal stellar structure with account of binary systems with compact comapnions. ...

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• Springer LINK:A&A-EE: Table of Contents Volume 333 Number 3 (1998)
• Springer LINK:A&A-EE: Table of Contents Volume 317 Number 3 (1997)
• Springer LINK:A&A-EE: Table of Contents Volume 319 Number 1 (1997)

D.Moss, R.Stepanov, T.G.Arshakian, R. Beck, M.Krause, D.Sokoloff, Multiscale magnetic fields in spiral galaxies: evolution and reversals, Astron. Astrophys., 537, A68, 13 pages (2012) . ... The effects of star-forming regions in galaxies need to be included when modelling the evolution of their magnetic fields, which can then be compared to future radio polarization observations. ... The injection of turbulent fields generates small-scale field structures. ...

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• Arshakian T. G., Stepanov R., Beck R., Krause M., Sokoloff D. Simulations of
• D.Sokoloff, Galaxy formation and evolution by Houjun Mo, Frank van den Bosch
• D.Sokoloff Galaxy formation and evolution by Houjun Mo, Frank van den Bosch and

... Sternberg Astronomical Institute , Moscow University . ... Present edition unites two parts of Catalogue of interacting galaxies by B.A.Vorontsov-Velyaminov: the first part (Part 1) containing 355 systems was published in 1959 [1] and the second one (Part 2) with 497 objects - in 1976 [2].Thus two published parts of Catalogue include 852 interacting systems. ... All new of them (1162 by number) were taken from the comments to the galaxies in Morphological catalogue by Vorontsov-Velyaminov et al.[ ...

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• IMCCE-SAI: Natural Satellites Service. Parameters and constants

Simulation of life inside Petri dish, where hypothetic unicellular organisms move and reproduce. ... They can't be changed while simulation is in progress Number of cells [1-10] - number of cells in dish at start of simulation Diameter of Petri dish [100-500] - defines the size of Petri dish Cell's lifetime [1-1000] - defines period of cell's life in dish Asexual(sexual) reproduction (on/off) - activates or disables chosen type of reproduction When you press "Submit" button, simulation is launched. ...

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... Among the methods of theoretical investigation of coordination compounds, molecular mechanics seems to be an optimal choice. However, conventional MM force fields typically do lack metal-related force field parameters. ... Let us calculate (MM) energy gradient for experimental structures using purely organic force field with no metal-dependent terms. ... In other words, thus calculated forces give an "imprint" for the derivation of metal-dependent forces. ...

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• Comparative Analysis of Intramolecular Parameters of Nitrocompounds:
• Optimization of Optical Scheme Parameters in Dual-Beam Thermal Lens...
• Photoacoustic detection of the parameters of laser vaporisation of amorphous

Dark matter annihilation in the Galaxy Veniamin Berezinsky Vyacheslav Dokuchaev Yury Eroshenko Institute for Nuclear Research, RAS, Moscow Laboratori Nazionali del Gran Sasso, Italy 14th Lomonosov Conference on Elementary Particle Physics DM clumps Standard cosmological scenario with an inflationary-produced primordial fluctuation sp ectrum Spike in the sp ectrum of p erturbations Clumps from isothermal fluctuations ... The solid curve shows the initial mass function. ...

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• http://nuclphys.sinp.msu.ru/conf/lpp14/210809/Di%20Bari.pdf

... All the galaxies are divided into 4 groups depending on the environment type; every subsample contains more than 10 galaxies. ... An effect of environments is seen both for the nuclei and for the bulges: if we consider the clusters (Virgo and Ursa Ma jor) and group centers as dense environments and the field and group periphery as sparse environments, then in the dense environments the stellar populations of S0s are in average older by 4­5 Gyr than in the sparse ones. ...

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• http://sn.sai.msu.ru/~sil/preprints/al292.pdf
• http://sn.sai.msu.ru/~sil/preprints/iau245sil.pdf
• http://sn.sai.msu.ru/~sil/preprints/iau254sil.pdf

... Field of research: Extragalactic astronomy. ... NASA Astrophysics Data System (ADS) Abstract Service . ... CADC Home Page . ... CCD Images of Galaxies . ... RUSSIAN LINKS . ... UA Astronomy Personal Home Page - Bill Keel . ... The Shape of the Rotation Curves of Edge-on Galaxies, by A.V.Zasov and A.V.Khoperskov, 2003. ... A Thickness of Stellar Discs, by A.V.Zasov, and D.V.Bizyaev, 2003 . Minimum Velocity Dispersion in Stable Stellar Disks, by A.V.Khoperskov, A.V.Zasov, and N.V.Tyurina, 2003 . ...

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Lomonosov Moscow State University , Skobeltsyn Institute of Nuclear Physics . Online Services | ... Links | ... Contacts | ... CDFE => Online Services => Nucleus Ground and Isomeric States Parameters Search Engine . The source of data is the Nuclear Wallet Cards database prepared and maintained by the USA NNDC. ... Show nuclear moments/deformations for selected nuclei . ... Metastable states: . ... If you have any questions, comments, and/or suggestions, please, contact . ...

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• CDFE => Online services => Chart of nucleus shape and size parameters
• CDFE => Online Services => Calculator and Graph Engine for Atomic Nuclei
• CDFE => Online Services => Relational ENSDF

... 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

... Mikhailov E.A. and Modyaev I.I. A problem connected with magnetic fields of galaxies is considered. ... These phenomena are characterized by dimensionless coefficients of the dynamo equations. ... The growth rates of statistical moments of the magnetic field are evaluated. ... The problem that has only a time dependence and the problem that has a spatial dependence are also considered. ... Keywords: galaxy magnetic fields, equations with random coefficients, dynamo theory, intermittency. ...

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• "A numerical method of parameter reconstruction in the FitzHugh-Nagumo and
• "An algorithm of assigning the force parameters to atoms of organic molecules
• "Influence of genetic algorithm parameters on the docking efficiency with the

... Next: Plane tab Up: Client Previous: Connection to a Server Contents Index . Figure 2.4: Scan parameters. STM mode of operation. ... AFM mode of operation. ... All scan parameters can be configures in Parameters window (pic. ... Client part of `` FemtoScan '' software allows to control microscope operating in three different scanning modes - tunneling mode(STM), atomic-force mode (AFM) and resonance atomic-force (RAFM). ... It(Z) tab (STM mode), F(Z) tab (AFM mode), D(Z) tab (RAFM mode). ...

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• Parameters of 3D Images
• Microscope Parameters Data
• Index

const int nvar_ is a number of independent physical parameters involved in the evaluation of squared matrix element. const int nfunc_ is a number of constrained parameters involved in the evaluation of squared matrix element. int calcFunc(void) calculates all constrained parameters for current values of independent ones. It returns 0 in the case of success, otherwise 1. int vinf_(int numvar, char *name, double *val) provides the information about parameters. ... It returns if , or otherwise. ...

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• [RU-NGI] GLUE2 parameters
• Independent parameters of the model
• Constraints between the parameters