... Visible predominantly from Earth's Southern Hemisphere , the LMC is the second closest galaxy , neighbor to the Small Magellanic Cloud , and one of eleven known dwarf galaxies that orbit our Milky Way Galaxy. The LMC is an irregular galaxy composed of a bar of older red stars, clouds of younger blue stars, and a bright red star forming region visible near the top of the above image called the Tarantula Nebula . ... Publications with keywords: Local Group of Galaxies - irregular galaxy - LMC . ...

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• Астронет > Neighboring Galaxy: The Large Magellanic Cloud
• M83: The Southern Pinwheel Galaxy from VLT
• Spiral Galaxy M83: The Southern Pinwheel

... 2000 February 22 . Neighboring Galaxy: The Large Magellanic Cloud . ... Explanation: The brightest galaxy visible from our own Milky Way Galaxy is the Large Magellanic Cloud (LMC). Visible predominantly from Earth's Southern Hemisphere , the LMC is the second closest galaxy , neighbor to the Small Magellanic Cloud , and one of eleven known dwarf galaxies that orbit our Milky Way Galaxy. ... The brightest supernova of modern times, SN1987A , occurred in the LMC . ... About APOD | ...

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• APOD: 2001 August 4 - Neighboring Galaxy: The Large Magellanic Cloud
• APOD: 2003 May 11 - M83: The Southern Pinwheel Galaxy from VLT
• APOD: 2005 December 18 - M83: The Southern Pinwheel Galaxy from VLT

Discover the cosmos! ... December 6, 1999 . M83: The Southern Pinwheel Galaxy from VLT . ... Explanation: M83 is one of the closest and brightest spiral galaxies on the sky. Visible with binoculars in the constellation of Hydra , majestic spiral arms have prompted its nickname as the Southern Pinwheel. Although discovered 250 years ago, only in this century was it appreciated that M83 was not a gas cloud but a barred spiral galaxy much like our own Milky Way Galaxy . ... About APOD > . ...

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• APOD: February 3, 1998 - A Magellanic Mural
• APOD: 2000 October 23 - Dwarf Elliptical Galaxy NGC 205 in the Local Group
• APOD: March 15, 1998 - Unusual M82: The Cigar Galaxy

Supernova 2000dk in NGC 382 . This page is devoted to information on Supernova 2000dk in NGC 382 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 Supernova links web page. ... We have a DSS Photometry reference image made by Odd Trondal. ... Odd Trondal's 2000dk page . ... LOSS image . ... 15.5 . ... vsnet-alert 5266 ] SN 2000dk in NGC 382 . ...

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• Supernova 1999gi in NGC 3184
• THE BRIGHT SUPERNOVA 1991T IN NGC 4527; AN AMATEURS PRESPECTIVE
• Multiple Supernovae in the same galaxy

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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• Shu F.H. - The Physical Universe: An Introduction to Astronomy :: Электронная
• Palen S. - Schaum's Outline of Astronomy :: Электронная библиотека
• Alloin D.M., Gieren W. - Stellar Candles for the Extragalactic Distance Scale

... As we have seen, evolutionary considerations based on our current understanding of massive binary systems lead to the conclusion that BH+PSR binaries must constitute a rather numerous subclass of all binary PSR ( 1 per 1000 isolated pulsars; Lipunov et al. , 1994b[ 124 ]). It seemed a priori that the binary radio pulsar PSR B0042-73   in the SMC (Kaspi et al., 1994[ 81 ]) could belong to one of these two classes. ... This means that such binary pulsars should be discovered in the near future. ...

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• Be/X-ray binaries and candidates
• Extragalactic Gravitational Wave Background
• Gravitational wave background from nearby galaxies

... MASTER Net is 56 square degrees per 1 exposition . ... 06 Dec 2015: GRB 151205B: MASTER-NET early optical observations GCN18665 . ... 18 Nov 2015: GRB 151118A: MASTER-NET optical observations GCN18613 . ... 12 Nov 2015: GRB 151112A: MASTER-NET optical limit GCN18591 . ... 07 Nov 2015: GRB 151107A: MASTER-NET optical observations GCN18565 . ... 31 Oct 2015: Five OTs detected by Global Robotic MASTER Net ATel8232 . ... 02 Oct 2015: GRB 151001B: MASTER-NET early optical observations GCN18380 . ...

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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
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... 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

... 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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... 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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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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• http://comet.sai.msu.ru/~gmr/prog_e.html
• IAC, Evolution of Galaxies, Conference
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... For the past years I have been working on the problem of synthesis of light curves of close binary systems, consisting of a normal star and a compact object (point object with fixed X-ray luminosity). ... Possible existence of a bright spot on the disk's lateral surface is taken into account. ... The last of then will be published in Gordon and Breach Publishers ( Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ... Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ...

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• Anatol Cherepashchuk
• Igor Antokhin
• Eugene Trunkovsky

... Invisible airwaves crackle with life Bright antenna bristle with the energy Emotional feedback on timeless wavelength Bearing a gift beyond price, almost free All this machinery making modern music Can still be open-hearted. ... You can choose a ready guide in some celestial voice. ... SONG: Different Strings Who's come to slay the dragon, Come to watch him fall? ... Tide Pools When the ebbing tide retreats Along the rocky shoreline, It leaves a trail of tidal pools In a short-lived galaxy. ...

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• http://crydee.sai.msu.ru/public/lyrics/cs-uwp/g/grateful.dead/throwing_stones
• http://crydee.sai.msu.ru/public/lyrics/cs-uwp/o/oldfield.mike/discovery.1
• http://crydee.sai.msu.ru/ftproot/pub/rec/music/lyrics/cs-uwp/c/clark.petula/misc.songs

... Consider the Virtual Brewery, a small company that brews, as the name indicates, virtual beer. To manage their business more efficiently, the virtual brewers want to network their computers, which all happen to be PCs running a bright and shiny 1.0. ... They run an Ethernet of their own. Quite naturally, the two companies want to link their networks once they are operational. As a first step, they want to set up a gateway host that forwards datagrams between the two subnets. ...

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• The boot process in closer look

Lab . Main page News People . ASA . Master . Master net Homepage . ... Lomonosov Moscow State University Sternberg Astronomical Institute . ... MASTER . ... Lomonosov (ShOK) . ... About Space Monitoring Laboratory, scientific directions, instruments, contacts . People, who work in lab . Latest news and news archive . ... Bright MASTER PSN discovery in UGC06716 galaxy ATel 3767 . ... All news ...

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... Opens another window with the same presentation loaded so you can work on more than one slide at a time. ... If enabled, formatting characters are visible; if disabled, they are not. View -> Help Lines . ... This guide-line will not print or display in the finished presentation, it is simply to help you align objects on screen. If this item is enabled, these help lines will be visible. ... Help lines work across slides, allowing you to align objects the same way across multiple slides. ...

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• Chapter€а15.€а Menus

... 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/ar1101.pdf
• http://sn.sai.msu.ru/~sil/preprints/mykukar.pdf
• http://sn.sai.msu.ru/~sil/preprints/pazh4036.pdf.gz

... We have compiled the Catalogue of extragalactic supernovae using the GCVS card catalogue. ... Doubtful (?), or rejected (-) SN 8 A1 --- RemFlag [*] The '*' indicates a remark in sn_rem.dat 10- 19 A10 --- Gal Parent galaxy designation 21- 22 I2 h RAh Right Ascension 1950 of Parent galaxy 23- 24 I2 min RAm Right Ascension 1950 (minutes) 25- 28 F4.1 s RAs Right Ascension 1950 (seconds) 29 A1 --- DE- Declination 1950 (sign) 30- 31 I2 deg DEd Declination 1950 of Parent ...

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• http://www.sai.msu.ru/gcvs/gcvs/v/readme
• Astronomical and Astrophysical Transactions

... История курсов . ... close this panel . ... Выпускной класс . Старшие классы . Младшие классы . ... Прием на курсы . ... График мероприятий . ... Телефоны, адреса . График работы . ... Приветствуем вас на сайте Общеуниверситетских подготовительных курсов.љ ... Обращаясь на курсы через форму "Задать вопрос", будьте внимательны при написании своего электронного адреса.љ . ... Сайт общеуниверситетских . подготовительных курсовљ . ...

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