... 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: February 3, 1998 - A Magellanic Mural
• APOD: February 22, 1999 - NGC 1316: After Galaxies Collide
• APOD: February 5, 1996 - COBE Dipole: Speeding Through the Universe

... February 23, 1998 . M104: The Sombrero Galaxy . Explanation: What's going on in the center of this spiral galaxy ? Named the Sombrero Galaxy for its hat-like resemblance, M104 features a prominent dust lane and a bright halo of stars and globular clusters . ... This X-ray emission coupled with unusually high central stellar speeds cause many astronomers to speculate that a black hole lies at the Sombrero's center - a black hole possibly a billion times the mass of our Sun. ...

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• APOD: 2004 February 11 - M64: The Sleeping Beauty Galaxy
• APOD: February 28, 1997 - Edge-On Spiral Galaxy NGC 891
• APOD: 2008 February 13 - Elliptical Galaxy NGC 1132

... The Andromeda Galaxy in Infrared . ... Credit: K. Gordon ( U. Arizona ), JPL-Caltech , NASA Explanation: What is the Andromeda galaxy really like? ... Astronomers trained the orbiting Spitzer Space Telescope at the Messier monster (M31) for over 18 hours, creating a mosaic that incorporated 11,000 separate exposures. ... Publications with keywords: M31 - Spitzer space telescope - infrared . Publications with words: M31 - Spitzer space telescope - infrared . ... Infrared Andromeda . ...

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• Abell 2744: Pandoras Cluster of Galaxies
• Elliptical Galaxy M87
• Barred Spiral Galaxy NGC 1300

... 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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• WORKSHOP "STELLAR ATMOSPHERES" "THE CHEMICAL AND DYNAMIC EVOLUTION OF STARS AND

Supernova Gallery The purpose of the Bright Supernovae web pages is to provide a place where people can find reference images of Supernovae. ... This is an RGB color image of Supernova 2003gs in NGC 936 Credit: Pablo Canadia . Used by permission. (click on image for full resolution) . ... This is an LRGB color image of Supernova 2003cg in NGC 3169 Credit: Pollux observatory . ... Credit: Nick Suntzeff Used by permission. (click on image for full resolution) . ... Credit: AURA/NOAO Image Library . ...

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• Multiple Supernovae in the same galaxy
• Supernova 2009js in NGC 918
• Supernova 2005ew in anonymous galaxy

Next: Ejectors in Massive Binary Previous: Artificial Galaxy: Full Matrix . The first version of the Scenario Machine was aimed especially at the simulation of massive binary star evolution. ... First, there is a large class of intermediate mass binaries (say, consisting initially of 8 + 5 solar masses) that can also produce NS and thus lead to the formation of a bright X-ray source. ... Next: Ejectors in Massive Binary Previous: Artificial Galaxy: Full Matrix Mike E. Prokhorov . ...

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• X-ray Luminosity Evolution
• Gravitational waves from supernova explosions
• Radiopulsars as Sources of Cosmic Rays

... 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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• List of Supernovae discovered by MASTER Net

... Kitchin C. - Galaxies in Turmoil: The Active and Starburst Galaxies and the Black Holes That Drive Them . ... Название: Galaxies in Turmoil: The Active and Starburst Galaxies and the Black Holes That Drive Them . ... Active galaxies (including Quasars, QSOs, Radio galaxies, BL Lacs, Blazars, LINERS, ULIRGS, Seyfert galaxies, Starburst galaxies, N galaxies, etc.) are a major field of current astronomical research. ... Электронная библиотека попечительского совета мехмата МГУ , 2004-2016 . ...

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• Keel W.C. - The Road to Galaxy Formation :: Электронная библиотека
• Eales S. - Origins: How the Planets, Stars, Galaxies, and the Universe Begane
• Schuecker P. (Ed), Boehringer H. - Heating Versus Cooling in Galaxies and

... 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/postbr1.pdf

... 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
• Division of the Galaxy and Variable Stars
• Anatoly V. Zasov

... 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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• Отдел внегалактической астрономии: ГАИШ Extra-galactic astronomy Group Student

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.Moss, D.Sokoloff, R.Beck, Ram pressure effects in the galactic plane and
• Moss D., Sokoloff D., Beck R., Ram pressure effects in the galactic plane and

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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• Different types of file
• rtftohtml Users Guide - 4 Special Processing
• rtftohtml Users Guide - 7 Nested Lists

16. Picornaviruses: discovering big in small

17. http://crydee.sai.msu.ru/ftproot/pub/rec/music/lyrics/cs-uwp/e/eloy/time.to.turn

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19. Russian Journal of Theriology

20. Laboratories: Laboratory for Comparative Ethology and Biocommunication: Results