... Credit: HST GRB Collaboration , STIS , HST , NASA Explanation: Do the powerful explosions known as gamma-ray bursts (GRBs) originate in galaxies? ... The diffuse object above is of particular interest because it appears to be the host galaxy of GRB 990123 . ... Are all host galaxies this strange? ... Publications with keywords: gamma-ray burst - host galaxy - GRB . Publications with words: gamma-ray burst - host galaxy - GRB . ... Gamma Ray Bursting . ... The Host Galaxies of Long Duration GRBs . ...

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• Астронет > GRB 990123 Host Galaxy Imaged
• Journal "Peremennye Zvezdy"
• M104: The Sombrero Galaxy

... 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: 2013 February 8 - NGC 6822: Barnard's Galaxy
• APOD: 2016 February 23 - A Supernova through Galaxy Dust
• APOD: February 28, 1997 - Edge-On Spiral Galaxy NGC 891

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

. This is the faintest SNe, at mag. 18.3, yet detected by my system. Mike Schwartz , Director . Tenagra Observatories, Ltd. Cottage Grove, OR 97424 . Back to Bright Supernovae . David Bishop Last modified: Tue Feb 16 08:42:58 EST 1999

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• Supernova 2000dx in UGC 1775
• Supernova 2005ch in anonymous
• Supernova 1999cl in M88

... 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
• Appenzeller I. (ed.), Habing H.J. (ed.), L?na P. (ed.) - Evolution of Galaxies
• Eales S. - Origins: How the Planets, Stars, Galaxies, and the Universe Begane

... 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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... 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
• Maidanak Lab page
• Division of the Galaxy and Variable Stars

... 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/postbr1.pdf
• http://sn.sai.msu.ru/~sil/preprints/ar578.pdf
• Olga Silchenko

... 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
• General Catalogue of Variable Stars: Vols I-III (the new electronic version).

... 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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Next: Gravitational Wave Background from Previous: Galactic Gravitational Wave Background . ... It is intuitively clear that at frequencies above the critical ones for our Galaxy, one will detect rare bright jerks produced by coalescing white dwarfs ? (at a rate of 1 per 100 year) and NS (at a rate of 1 per - year) in our Galaxy, against a background of the extragalactic stochastic GW. ... Firstly we consider GWB from close individual galaxies, and then will discuss overall extragalactic GWB. ...

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• Massive X-ray Binaries
• X-ray Luminosity Evolution
• Gravitational wave background from nearby galaxies

TWiki has a very simple text formatting shorthand . ... If a discussion is going on: . ... add your WikiName and the date at the end. ... Main.TWikiGuest - 10 Apr 2016 . ... if you'd like to use an initial, use a link with label. ... Main.TWikiGuest][ZXQ]] - 10 Apr 2016 . A good format for a new topic is "dissertation followed by discussion": . ... TWiki is intended for world-wide use, and an internationally understood date format like 01 Sep 2016 or 2016-09-01 is preferred. ...

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• GoodStyle - TWiki - TWiki

Lomonosov project . ... Scientific goals . ... Gamma-bursts . ... One of the most mysterious phenomena in he Universe is gamma-burst ? ... These phenomena being the most powerful in the Universe occur not only in gamma-range, but also in optic and UV. Gamma-bursts were discovered in 60s years of 2oth century but only after 1997 were the optic emission of gamma-bursts was detected for the first time  it became clear that we deal with the most powerful processes in the Universe. ... Device BDRG . ...

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• Collaboration | Университетский спутник "Ломоносов"
• Transient luminous events | Университетский спутник "Ломоносов"
• News | Университетский спутник "Ломоносов"

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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• IAC, Evolution of Galaxies, Conference

... High Brightness RTM . ... Fig.1a: 70-MeV pulsed race-track microtron . Many applications require compact, inexpensive and efficient source of electron beam in energy range 10-100 MeV. ... Beam is focused by accelerating structure, which acts as RF quadrupole singlet, quadrupole triplets (12) installed at the even orbits return path and by electromagnet quadrupole singlet (9) installed at common axis. ... Fig.1b: 70-MeV RTM Schematic . ... Energy gain: 4.8 MeV / orbit . Orbits: 14 . ...

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Центр коллективного пользования . МГУ им. М.В. Ломоносова . ... Главная страница . О центре . ... Уже несколько лет в МГУ действует Центр коллективного пользования, объединивший передовые лаборатории естественнонаучных факультетов МГУ, в распоряжении которых имеется самое современное оборудование. ... Центр коллективного пользования МГУ им. М.В. Ломоносова, 2009 . ...

18. Theory as a Lighthouse in the Electrochemical Ocean

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

20. GoodStyle < System < Foswiki