The divisity of galaxies. The galaxies are the giant (to hundred of billions of stars) star systems, where the stars are connected by gravitation laws with each other. ... Ther galaxy NGC 3031 . ... Each spiral galaxy has a core a flat disk where the spiral brancher locate. The stars and interstellar substance of spiral galaxies rotate around the core. ... In normal galaxies, such as our Galaxy, the great brightness of the core is accounted for the high concentration of stars. ...

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• irasphotoe
• gershele

... Main page News People . ASA . Master . Master net Homepage . ... MASTER . ... About Space Monitoring Laboratory, scientific directions, instruments, contacts . ... Latest news and news archive . ... 08.11.2011 . ... All news ...

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... INSTRUMENT: SurveyCam FILTERS: Stromgren uvby, 2" square COMMENTS: remote observations are expected BRIEF SCIENCE JUSTIFICATION: Last decade numerous faint structures at the periphery of regular galaxies, as arcs, tails, or streams, have been discovered (see e.g. Martinez-Delgado et al., ... The broad-band photometry is used for observing the faint structures, but it does not allow to break the age-metallicity degeneracy efficiently. ... The standard Stromgren set is available at APO. ... 2014). ...

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• http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_jan2016/AS06.html
• http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_apr2016/AS06.html
• TUI:Guiding:User's Guide

... 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.su/gcvs/gcvs/v/readme

... Ciel Espace, le magazine qui vous guide toujours plus loin . ... des pages consacr†ées †à la publication de vos photos Mais c'est aussi une vraie communaut†é avec laquelle partager votre passion et nourrir votre curiosit†é. Accueil Mati†ère noire : une observation d†éfie les astronomes . ... A la une . ... En effet, selon les mod†èles th†éoriques, les concentrations de mati†ère noire sont les lieux o†µ naissent les galaxies. ... Une mati†ère noire au comportement ordinaire ? ... Etat du ciel . ...

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• Toute la violence dòÀÙun amas de galaxies | Ciel et Espace
• Les galaxies barr†ées sont moribondes | Ciel et Espace
• Une collision de galaxies en 3D | Ciel et Espace

... Authors: Sjoert van Velzen et al. arxiv:1511.07746 Ïÿòü íîâûõ áûñòðûõ ðàäèîâñïëåñêîâ ïî äàííûì îáçîðà HTRU íà âûñîêèõ øèðîòàõ: ïåðâûå óêàçàíèÿ íà äâóõêîìïîíåíòíûå âñïëåñêè (Five new Fast Radio Bursts from the HTRU high latitude survey: first evidence for two-component bursts) . Authors: D. J. Champion et al. arxiv:1511.00704 Áûñòðîðàñòóùèå òðàíçèåíòû â ïðîìåæóòêå ìåæäó ñâåðõíîâûìè è óëüòðàìîùíûìè ñâåðõíîâûìè (Rapidly Rising Transients in the Supernova - Superluminous Supernova Gap) . ...

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• http://xray.sai.msu.ru/~polar/sci_rev/0308.html
• http://xray.sai.msu.ru/~polar/sci_rev/1307.html
• Free Virtual Galaxy 1.0b

... The Co­Addition Technique Applied to Images of Galaxy Cores W. W. Zeilinger Institut f˜ur Astronomie, University of Vienna, T˜urkenschanzstraúe 17, A­1180 Wien, Austria P. Crane, P. GrosbÜl and A. Renzini European Southern Observatory, Karl­Schwarzschild Straúe 2, D­85748 Garching, Germany Abstract. ... One may therefore take full advantage of the high resolution FOC images by co­adding them with (high signal­to­noise) ground­ based data. ... References Crane, P. et al. ...

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• ESLAB 2007
• The Structure and Composition of High Redshift Radio Galaxies
• A Color Analysis of NICMOS Parallel Observations

... 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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... About ATMoB . ... The Observing Committee is starting an Observing Awards Program to promote observing among the membership of the Amateur Telescope Makers of Boston. ... Participant must be a current member of the Amateur Telescope Makers of Boston . ... To qualify for your Observing Award Certificate, turn in your worksheet and drawings to an ATMoB Observing Committee member or observing@atmob.org . ... This Excel sheet has useful macros. ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

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• Amateur Telescope Makers of Boston

... The main field of my investigations is stellar spectrophotometry. As a result of scientific activity of our group spectrophotometric catalog was created including energy distribution data on 900 stars in the range 3200-7600AA and 250 stars in the range 6000-10800AA (Voloshina et al., Spectrophotometry of Bright Stars, ed. I.N.Glushneva, 1982, Moscow, Nauka, in Russian). ...

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... arXiv.org . astro-ph . ... We fit the near-infrared to radio spectral energy distributions of 30 luminous and ultra-luminous infrared galaxies with pure starburst models or models that include both starburst and AGN components to determine important physical parameters for this population of objects. In particular we constrain the optical depth towards the luminosity source, the star formation rate, the star formation efficiency and the AGN fraction. ...

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... In the table given at a separate sheet enumerate in growing order (from 1 to 13) the size and the mass of each object: Milky Way Galaxy, Andromeda Galaxy, Neutron star, Electron, Mercury, The first satellite "Sputnik I", Venus, Pluto, Proton, Red dwarf, Black cat, White (Polar) bear, the Sun. ... Star setting. ... Comet Lovejoy. ... Radio- (operating wavelength is about 21 cm) and optical (operating in the light visible to the naked eye) telescopes have been used to study an astrophysical object. ...

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• III International Astronomy Olympiad, Problems to solve

... Æåíñêàÿ êóðòêà èç íàòóðàëüíîé êîæè . ... Áðåíä: Samsung, Òèï: ÷àñû, Ñîâìåñòèìîñòü: âçàèìîäåéñòâèå ñ Android, Îñîáåííîñòè: ìîíèòîðèíã ôèçè÷åñêîé àêòèâíîñòè . ... Êàáåëü ñîåäèíèòåëüíûé 1.5ì Hama Cinch Digital RCA (M) - RCA (M) ïîçîëî÷åííûå êîíòàêòû ÷åðíûé 122266 - HAMA - HAMA . ...

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• ×åõîë IT BAGGAGE äëÿ ïëàíøåòà SAMSUNG Galaxy Tab Pro 10.1 èñêóññòâåííàÿ êîæà
• Samsung SM-G355H Galaxy Core 2 Duos, White - Samsung - Samsung SM-G355HZWDSER
• G-case Slim Premium ÷åõîë äëÿ Samsung Galaxy Note 3, Blue - G-Case - G-Case

P.N. Lebedev Physical Institute Astro Space Center Russian Academy of Sciences S.A. Lavochkin Association, Roscosmos RADIOASTRON The Ground ­ Space Interferometer: radio telescope much larger than the Earth The Spectr-R Project http://www.asc.rssi.ru/ radioastron / High- Resolution HI 21 cm Mosaic of M 33 galaxy GENERAL OUTLINE The RadioAstron ... Such forecast could be used to prepare a long time-scale schedule of scientific observations. ...

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• MILLIMETRON
• MEMORANDUM

... Director of the RAS ISR . RAS Academician . ... Astrophysics module Kvant of the orbital complex Mir launched in 1987 contains the largest on the station complex of the scientific equipment named the orbital observatory Roentgen. Observatory Roentgen consists of 4 X-ray telescopes, jointly exceeding the range of energies from 2 to 800 keV. ... Among the most significant results that were received in the observatory Roentgen are: . ... measurement of the periods of 9 X-ray pulsars; . ...

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... Courtesy of NASA/ESA Observation data (J2000 epoch) Constellation Right ascension Declination Redshift Distance Type Serpens Caput 15h 17m 14.4s[] +21° 35 08[] 12,740±50 km/s[][1] 600±30 Mly (183±8 Mpc)[1] SA0(r) [citation needed ] [a] Apparent dimensions (V) 0.28 â 0.28[] Apparent magnitude (V) 16.0[] Notable features Ring galaxy Other designations PGC 54559,[] PRC D-51[] See also: Galaxy, List of galaxies Hoag's Object is a non-typical galaxy of the type known as a ring galaxy. ...

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• Distribution (ImageJ API)

Comment on J0627-3529 . We have detected the core of an FR-I object and early-type galaxy (Venturi et al. 1995). The core is 0.54 Jy at 2.3 GHz on the Parkes-Tidbinbilla baseline (Morganti et al. 1997) and 0.6 Jy at 5 GHz (VLA data, Ekers et al. (1989) and Morganti, Killeen & Tadhunter (1993)). The VLBA image at 2.3 GHz with the resolution of 15x9 mas shows a "core-jet" structure, with the core brightness of 494 mJy/beam (Venturi et al. ...

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... NGC 4631 Whale galaxy (Caldwell 32) - ñïèðàëüíàÿ ãàëàêòèêà ñ ïåðåìû÷êîé Êèò (Arp 281) â ñîçâåçäèè Ãîí÷èõ Ïñîâ (Canes Venatici) .. ... Ïðîñìîòð ïîëíîé âåðñèè : NGC 4631 Whale galaxy (Caldwell 32) - ñïèðàëüíàÿ ãàëàêòèêà ñ ïåðåìû÷êîé Êèò (Arp 281) â ñîçâåçäèè Ãîí÷èõ Ïñîâ (Canes Venatici) .. ... NGC 4631 Whale galaxy (Caldwell 32) - ñïèðàëüíàÿ ãàëàêòèêà ñ ïåðåìû÷êîé Êèò (Arp 281) â ñîçâåçäèè Ãîí÷èå Ïñû (Canes Venatici (http://www.starlab.ru/showpost.php?p=178940&postcount=721)) .. ...

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• Îáùàÿ Àñòðîíîìè÷åñêàÿ Êîíôåðåíöèÿ - Ïîêàçàòü ñîîáùåíèå îòäåëüíî - NGC 4631
• NGC 6240 Starfish Galaxy - óëüòðàëþìèíåñöåíòíàÿ èíôðàêðàñíàÿ ãàëàêòèêà (ULIRG)
• Messier 101 Pinwheel Galaxy (M101) - ñïèðàëüíàÿ ãàëàêòèêà NGC 5457 â ñîçâåçäèè

... The dynamics of silicate and graphite particles with radii of (0.1-2) 10 -5 cm in the vicinity of the Milky Way is considered. The equation of motion of dust grains is integrated with gravitational attraction, radiation pressure, gas drag, and dust destruction taken into account. The effect of other factors on the motion of grains are discussed. ... Dust is swept out of the Galaxy by radiation pressure from stars at a rate of 0.04 M o yr -1 . ...

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• Future of the Galaxy
• Project: PAHs
• Gradients in Disk Galaxies

Microsymposium 38, MS083, 2003 (A4 format) MERCURY: LOCAL VARIATIONS OF THE PHOTOMETRIC RELIEF. ... Because of trajectory and pointing angle constraints the planet could be observed from Mariner 10 only over a small range of phase angles between about 75o and 110o. Therefore the photometric investigations are restricted to measuring the distribution of brightness on the Mercurian disk. ... Raw versions of real-time processing pictures FDS 0000984 and FDS 0000986 were used (images 196 and 202). ...

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• http://selena.sai.msu.ru/Shev/Publications/m44_76_sinitsin_shevchenko.pdf
• http://selena.sai.msu.ru/Pug/Publications/Pugacheva%20LPS%2041.pdf
• http://selena.sai.msu.ru/Shev/Publications/m44_75_shevchenko_etal.pdf