... Dark Matter Ring Modeled around Galaxy Cluster CL0024+17 . ... It is the relatively weak distortions of the many distant faint blue galaxies all over the image, however, that indicates the existence of the dark matter ring. ... A hypothesis for the formation of the huge dark matter ring holds that it is a transient feature formed when galaxy cluster CL0024+17 collided with another cluster of galaxies about one billion years ago, leaving a ring similar to when a rock is thrown in a pond. ...

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• APOD: 2011 June 29 - Abell 2744: Pandora's Cluster of Galaxies
• APOD: 2001 February 22 - 3C294: Distant X Ray Galaxy Cluster
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... The Hydra Cluster of Galaxies . ... Most of a cluster's mass , however, appears to be in a form too dark to see , as analyses of the distribution of X-ray light , gravitational lensing , and internal motions indicate. ... The Hydra Cluster of Galaxies, named for its home constellation , spans about ten million light years . ... Publications with keywords: Hydra - cluster of galaxies . Publications with words: Hydra - cluster of galaxies . ... Illusion and Evolution in Galaxy Cluster Abell 2667 . ...

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• Galaxy Cluster Magnifies Distant Supernova
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... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. 2000 February 28 . The Sombrero Galaxy from VLT . ... FORS1 , VLT ANTU , ESO . ... Reasons include the Sombrero 's unusually large and extended central bulge of stars, and dark prominent dust lanes that appear in a disk that we see nearly edge-on. Billions of old stars cause the diffuse glow of the extended central bulge. ... About APOD | ...

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• APOD: 2000 August 18 - X-Rays From Antennae Galaxies
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• APOD: July 9, 1999 - NGC 7789: Galactic Star Cluster

Page 1 I*M*P*R*S on ASTROPHYSICS at LMU Munich Astrophysics Introductory Course Lecture given by: Ralf Bender and Roberto Saglia in collaboration with: Chris Botzler, Andre Crusius-WДtzel, Niv Drory, Georg Feulner ... , Ulrich Hopp, Claudia Maraston, Michael Matthias, Jan Snigula, Daniel Thomas Powerpoint version with the help of Hanna Kotarba Fall 2007 IMPRS Astrophysics Introductory Course Fall 2007 ... IMPRS Astrophysics Introductory Course Fall 2007 Page 17 11.2. ...

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• http://lnfm1.sai.msu.ru/~gusev/catalog/readme
• Division of the Galaxy and Variable Stars
• Yuri Nicolaevich Efremov - My Home Page

... Previous message: [Comphep-common] Passing compHEP 4.4.3 events to Pythia (fwd) . Next message: [Comphep-common] [Fwd: Re: [Comphep-devel] [Fwd: uncertainty on 2l invariant mass distributions of ZZ production]] . ... Which are the most relevant sources of uncertainty in the shape of dilepton invariant mass distribution between 10 and 60 GeV, that is, which parameters in CompHEP should we vary to get a estimate of the uncertainty ? ... More information about the Comphep-common mailing list . ...

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• [Comphep-common] [Fwd: Re: [Comphep-devel] [Fwd: uncertainty on 2l invariant
• fc3:cluster:thep02 [THEP]
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Электронная библиотека Попечительского совета . ... Raine D.J. - The Isotropic Universe: An Introduction to Cosmology . ... Название: The Isotropic Universe: An Introduction to Cosmology . Автор: Raine D.J. Аннотация: . An introduction to modern ideas on cosmology and on the physical basis of the general theory of relativity. ... Anisotropic universes 6 196 . Anisotropic universes, classification of 202 . ... Электронная библиотека попечительского совета мехмата МГУ , 2004-2016 . ...

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• Appenzeller I. (ed.), Habing H.J. (ed.), L?na P. (ed.) - Evolution of Galaxies
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... Обучение . ... Проводится запись на очные курсы СУНЦ МГУ на 2011-12 учебный год . ... СУНЦ МГУ школа им. А.Н.Колмогорова . ...

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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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... Keeping Time . ... The date command shows the current date and time. 1] For example: $ date Sun Jul 14 21:53:41 EET DST 1996 $ That time is Sunday, 14th of July, 1996 , at about ten before ten at the evening, in the time zone called ``EET DST'' (which might be East European Daylight Savings Time ). date can also show the univeral time : $ date -u Sun Jul 14 18:53:42 UTC 1996 Sun Jul 14 18:53:42 UTC 1996 $ date is also used to set the kernel's software clock : # ...

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... ONLY include the controls you are actually using. ... only used if > -100 !Profile_xmax = 1.2 !-101 ! ... only used if > -100 Profile_other_ymax = -101 ! ... step number. negative means use default. ... negative means use same value as for window CONV_file_aspect_ratio = -1 ! negative means use same value as for window ! ... negative means use same value as for window Surf_Hist_file_aspect_ratio = -1 ! ... negative means use same value as for window Power_file_aspect_ratio = -1 ! ...

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Supernova 1999cl in M88 . This page is devoted to information on Supernova 1999cl in M88 Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main supernova page. Information on the original web pages for many of these images can be found on the Supernova links web page. ... M1 Supernova Search has a 1999cl page . ... Pedro Re' Animated gif image . ... DAX Observatory . ... vsnet-obs 21040 ] (fwd) Observation of Supernova 1999cl in M88 . ...

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... Using the CFBDSIR wide field survey for brown dwarfs, we identified CFBDSIRJ214947.2-040308.9, a late T dwarf with atypically red J-Ks colour. ... SN 2009ip in NGC 7259 Electronic Telegram No. ... 7.09, [19.0; 2009 Aug. ... Accepted for publication in MNRAS Subjects: High Energy Astrophysical Phenomena (astro-ph.HE) The jet opening angle theta_jet and the bulk Lorentz factor Gamma_0 are crucial parameters for the computation of the energetics of Gamma Ray Bursts (GRBs). ...

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THE ARGUMENT AGAINST LONG EXTRAGALACTIC DISTANCE SCALE Gaseous discs of S0 -- Sd galaxies appears to be gravitationally stable or close to stability. Dependence of the gravitational stability parameter of gaseous disc $M_g/M_c$ upon the color index $(B-V)^0_T$ which reflects a relative number of young stars, is found. Here $M_g$ is total mass of gas in a galaxy, $M_c$ - mass of gas which corresponds to marginal stability of gaseous disc at distances from center. ...

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• Examples of showing the value of variables
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... All contacts alignment . ... Blue background means a contact with backbone phosphate. ... HBond with major groove + contact through a molecule of water with backbone phosphate; . ... contacts through water molecules both with backbone phosphate and major groove; . ... HBond with major groove + contacts through water molecules both with backbone phosphate and major groove; . ... HBond with major groove + engagement in hydrophobic cluster + contact through a molecule of water with backbone phosphate; ...

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• Hydrophobic clusters
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. Kudryashov S.I. , Zorov N.B. Mendeleev Communications, p. 178 (1998). Abstract . The electric probe procedure developed here has made it possible to detect for the first time large cluster ions, the products of spinodal decomposition of the laser-induced labile state of the liquid phase of carbon, with a size up to a million atoms and relative content in the mass distribution of the order of ppm. Laboratory of Laser Diagnostics

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• Moscow University Chemistry Bulletin Vol. 44, No. 2, P. 108 (2003)
• Moscow University Chemistry Bulletin Vol. 44, No. 3, P. 183 (2003)
• Time-of-flight mass spectroscopy detection of new elemental and mixed small

Twilight observations with MASS/DIMM B. Safonov Sternberg Astronomical Institute Moscow State University Comprehensive Characterization of Astronomical Sites, 2010 B. Safonov (Moscow State University) Twilight observations with MASS/DIMM SITE 2010 1 / 17 Why observe in twilight with MASS/DIMM? ... ASM includes 3 devices sensitive to background: guider, DIMM and MASS. B. Safonov (Moscow State University) Twilight observations with MASS/DIMM SITE 2010 2 / 17 Background in guider. ...

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COMPARISON OF CLUSTERING ALGORITHMS FOR SPEAKER IDENTIFICATION Nikolay Lubimov, Evgeny Mikheev, Alexey Lukin Moscow Lomonosov State University, Moscow, Russia In this paper we consider the problem of text-independent speaker identification that refers to acoustic recognition research. ... We have performed the comparison of different clustering methods for speaker identification: the standard K-means clustering, K-means++, Linde-Buzo-Gray, Fuzzy C-means, and Gustafson-Kessel algorithms. ...

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arxiv:1307.8241 Кривая вращенияи распределение массы в центре Галактики --- от черной дыры до самых до окраин (Rotation Curve and Mass Distribution in the Galactic Center --- From Black Hole to Entire Galaxy) . Authors: Yoshiaki Sofue . ... Authors: D. Thornton et al. arxiv:1307.2944 Архив экзопланет NASA: Данные и инструменты для экзопланетных исследований (The NASA Exoplanet Archive: Data and Tools for Exoplanet Research) . ... обзор arxiv:1307.0041 Галактическая археология. ...

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... How can I write fixed font text? ... To prevent auto-linking - say you want to enter a word like JavaScript (the proper spelling!) - prefix the WikiStyleWord with the special TWiki HTML tag <nop> : . ... TWiki interprets text as HTML, so you can use the preformatted HTML text option to keep the new line of text as is. ... The pre tag is standard HTML; verbatim is a special TWiki tag that also forces text to fixed font mode, and also prevents other tags and TWiki shortcuts from being expanded. ...

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... 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. ...

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