... 2008 September 17 . MACSJ0025: Two Giant Galaxy Clusters Collide . ... Explanation: What happens when two of the largest objects in the universe collide? ... In the case of MACSJ0025.4-1222 , two huge clusters of galaxies have been found slowly colliding over hundreds of millions of years, and the result has been imaged by both the Hubble Space Telescope in visible light and the Chandra Space Telescope in X-ray light . ... Note: Free Astronomy Course Taught Online by an APOD Editor . ...

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• APOD: September 17, 1995 - Thousands of Coma Cluster Galaxies
• APOD Index - Galaxies: Clusters of Galaxies
• APOD: 2009 September 21 - Abell 370: Galaxy Cluster Gravitational Lens

... A dwarf elliptical galaxy, M110 ( aka NGC 205 ) is actually a bright satellite of the large spiral galaxy Andromeda , making M110 a fellow member of the local group of galaxies. ... Publications with keywords: M 110 - NGC 205 - dwarf galaxy - Local Group of Galaxies . Publications with words: M 110 - NGC 205 - dwarf galaxy - Local Group of Galaxies . ... Bright Star Regulus near the Leo I Dwarf Galaxy . ... M31: The Andromeda Galaxy . NGC 1569: Starburst in a Dwarf Irregular Galaxy . ...

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• Thousands of Coma Cluster Galaxies
• MACSJ0025: Two Giant Galaxy Clusters Collide
• The Coma Cluster of Galaxies

... December 13, 1997 . The Coma Cluster of Galaxies . ... The Coma Cluster of Galaxies pictured is one of the densest clusters known - it contains thousands of galaxies . Each of these galaxies house billions of stars - just as our own Milky Way Galaxy does. ... In fact, the Coma Cluster is so big it takes light millions of years just to go from one side to the other! Most galaxies in Coma and other clusters are ellipticals , while most galaxies outside of clusters are spirals . ...

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• APOD: September 22, 1998 - M61: Virgo Spiral Galaxy
• APOD: September 17, 1999 - M3: Half A Million Stars
• APOD: May 3, 1997 - Giant Cluster Bends, Breaks Galaxy Images

Электронная библиотека Попечительского совета . ... Kaastra J. - Clusters of Galaxies: Beyond the Thermal View . ... Название: Clusters of Galaxies: Beyond the Thermal View . Автор: Kaastra J. Язык: . ... Электронная библиотека попечительского совета мехмата МГУ , 2004-2016 . ...

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• Schuecker P. (Ed), Boehringer H. - Heating Versus Cooling in Galaxies and
• Stebbins J. - Absorption and Space Reddening in the Galaxy as Shown by the
• van Paradijs J., Bleeker J.A.M. - X-Ray Spectroscopy in Astrophysics ::

Alexey Rastorguev's links to DataBases and Catalogs: . ... Open Clusters and Galactic Structure База данных и каталог рассеянных скоплений Галактики . ... USNO: Astronomical Applications Каталоги и базы данных - проекты Морской Обсерватории США . ... HST Science Data Archive Архив данных HST . CFHT Data Archive Архив данных CFHT . ... USNO Recommended Star Catalogs (Zacharias N. et al.) ... USNO Star Catalogs Каталоги USNO . ... USNO-B1.0 Catalog Астрометрический каталог USNO-B1.0 . ...

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

... Structure of Data . ... Catalog . ... In SAI OCL Catalog, we introduce our work on investigation of the Milky Way system of open star clusters. The main goal of our study is a search for new clusters using huge surveys. 168 new clusters have been already discovered by us using J,H,Ks data from 2MASS point source catalog. ... For 141 new clusters, we found their physical parameters using J,H,Ks data from 2MASS catalog and, for a number of clusters, our UBVRI CCD observational magnitudes. ...

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• SAI OCL Catalog Publications
• SAI OCL Catalog Structure
• SAI OCL Catalog Description

... 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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• Absolute proper motions of open clusters

D.Moss, D.Sokoloff, R.Beck, Ram pressure effects in the galactic plane and galactic dynamos in the no-z approximation, Astron. Astrophys., 544, A5, 4 pages, 2012 . ... To isolate the leading physical effects, we exploit a simple dynamo model that can describe relevant effects. ... Any determination of galactic motion through the cluster medium from observational data needs to take the effects of dynamo action into account. ...

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• Moss D., Sokoloff D., Beck R., Ram pressure effects in the galactic plane and
• Beck R., Frick P., Stepanov R., Sokoloff D. Recognizing magnetic structures by
• Beck R., Frick P., Stepanov, R., Sokoloff D. Recognizing magnetic structures by

Find Similar Abstracts . ... The formation of galaxies in Friedmannian universes . ... 00/1974 . ... ASTROPHYSICS, COSMOLOGY, GALACTIC CLUSTERS, GALACTIC EVOLUTION, GRAVITATION THEORY, DENSITY DISTRIBUTION, GALACTIC ROTATION, GAS HEATING, GAS IONIZATION, PERTURBATION THEORY, TEMPERATURE DISTRIBUTION . ... Use: Authors Title Abstract Text Text Query with Keywords Return: Query Results Query Form Database: Astronomy Instrumentation Physics and Geophysics ABSTRACT QUERY USER FEEDBACK HELP ...

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• Gravitational Wave Background from Individual Galaxies
• Structure of the Galaxy
• Be/X-ray binaries and candidates

... This form lets you to produce a list of hydrophobic clusters in a PDB file specified by user. Enter a 4-letter PDB code, e.g.: 1apl : . Search clusters: . ... between chains . Contacts between chains . Set #1 . ... Enter your e-mail here (optional): . ... List of atoms Strict Wide . Chains filter (1-20:A) . Show clusters not smaller than atoms . User data file in PDB format . ...

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• ETS_water_bridges
• Inquiry information || Distances
• About COGs

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 319 Number 1 (1997)
• Springer LINK:A&A-EE: Table of Contents Volume 333 Number 3 (1998)
• Springer LINK:A&A-EE: Table of Contents Volume 318 Number 1 (1997)

. Domain architecture . Protein role . Number of proteins . Clusters that contain proteins with the same domain architecture . SseC . Unknown . 1 proteins . 44 73 39 68 128 40

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• Cluster 12
• Cluster 128
• Cluster 13

... Moscow Lomonosov State University . ... Consider an open network consisting of N nodes (stations) and V(N) cars, which circulate among the stations. The network is divided into n clusters. ... Cluster j contains d N j N stations, Е j = 1 n d N j = 1. ... Later j and v denote cluster numbers and they take values from 1 to n. The arrival process to a station of cluster j is a Poisson one with the rate l j . ... The destination station in the cluster v is chosen uniformly. ...

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. of Lomonosov Moscow State University, . Russia . GCVS Research Group . Catalogues of Variable Stars . Future Prospects of Variable-Star Catalogues . B.V. Kukarkin Centenary Conference: Variable Stars, the Galactic Halo and Galaxy formation (VS-Halo) . What's new . Recent publications . Digitization of Moscow Plate Archive . The "Peremennye Zvezdy" (Variable Stars) journal . Send questions and comments to Olga Durlevich .

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• Конференции сайта АстрО

... 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 4ґ5 Gyr than in the sparse ones. ...

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• http://sn.sai.msu.ru/~sil/preprints/mykukar.pdf
• http://sn.sai.msu.ru/~sil/preprints/my_an.pdf
• http://sn.sai.msu.ru/~sil/preprints/iau245sil.pdf

Выберите категорию обращения: Общие вопросы Отчеты Рейтинги Диссертационные советы Конкурсы Ввод данных Структура организаций Пользователи Проблемы с регистрацией\входом в систему . ... Войти в систему . ... Mel'nik A.M. , Rautiainen P. , Glushkova E.V. , Dambis A.K. в журнале Astrophysics and Space Science , издательство Kluwer Academic Publishers (Netherlands) , том 361, ? ... Melnik A.M. , Rautiainen P. , Berdnikov L.N. , Dambis A.K. , Rastorguev A.S. в журнале VizieR Online Data Catalog . ...

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• Vlasyuk V.V. - сотрудник | ИСТИНА - Интеллектуальная Система Тематического
• Zeitschrift Fur Physik D-Atoms Molecules and Clusters - журнал | ИСТИНА -
• Spiridonova O.I. - сотрудник | ИСТИНА - Интеллектуальная Система Тематического

... Spinodal decay of the laser-induced labile liquid state of a carbon was observed by TOF MS and the electric probe technique as a threshold-like appearance of the carbon giant cluster ions ( sized from 50 up to million atoms ) at 0.3 GW/cm2 power density value besides the small cluster ions (C1-25) detected in mass spectra over the whole power density range. ...

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• Moscow University Chemistry Bulletin Vol. 50, No. 1, P. 9 (2009)
• Moscow University Chemistry Bulletin Vol. 51, No. 5, P. 339 (2010)
• The mechanism of giant carbon cluster formation at laser destruction of

Supernova 2002bu in NGC 4242 . This page is devoted to information on Supernova 2002bu in NGC 4242 Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . Information on the original web pages for many of these images can be found on the updates and links web pages. This is a type IIn supernova found in a galaxy which is in Canes Venatici. ... Mag . ... 2002/03/28.26 . ... A Leroy image . ... SUPERNOVA 2002bu IN NGC 4242 . ...

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• Supernova 1999gi in NGC 3184
• Multiple Supernovae in the same galaxy
• Supernova 2000cz in IC 1535

... Difference between workstation clusters and MPPs . Up: Special features of different systems Next: Checking your machines list Previous: Special features of different systems . ... In contrast, workstation clusters require that each process in a parallel job be started individually, though programs to help start these processes exist (see Using the secure server below). ... Using heterogeneous clusters is discussed below.) ... Центры . ...

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• Special features of different systems | PARALLEL.RU -
• 
  <tt> mpirun
  </tt>, a Portable Startup Script | PARALLEL.RU -

... 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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• CLEO: USER & ADMIN-FRIENDLY CLUSTER BATCH SYSTEM | Moscow University
• APPLICATIONS: Astronomy | Moscow University Supercomputing Center
• Welcome to HPC.MSU.RU! | Moscow University Supercomputing Center