The radial distribution of metallicity of star-forming galaxies in a galaxy cluster can inform us about the mass assembly and enrichment history of the galaxy cluster. ... Both galaxy clusters are cool-core clusters at redshift z т?? ... The gas-phase metallicity of star- forming galaxies in MACS1115+01 exhibit anti-correlation with projected distance т??0.15 ТБ 0.08 dex/Mpc, whereas the radial metallicity distribution of RXJ1532+30 is statistically flat (т??0.09 ТБ 0.12 dex/Mpc). ...

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• http://www.mso.anu.edu.au/pfrancis/roleplay/ziggy/model_answer2.doc
• http://www.mso.anu.edu.au/pfrancis/roleplay/ziggy/model_answer2.pdf
• Julie Banfield | Astronomer

... Visible Distribution of Galaxies. ... Features of Elliptical, Lens-Shaped, Spiral and Irregular Galaxies. Galaxies with Bar. ... Distribution of Surface Brightness of Surface and Spiral Galaxies. ... Color Characteristics of Galaxies. ... Methods of Galaxies' Mass Determination. ... Hidden Mass of Spiral Galaxies. ... Features of Dark Matter Distribution in E and SO Galaxies. ... The Whole Number of Galaxies and Their Density by the Results of Observation on the 'Hubble' Space Telescope. ...

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• Stellar Astronomy

... Future seminars . P a s t seminars . Seminar council . Stability of cold fronts in clusters of galaxies " . E. Churazov (IKI, MPA) . ... One of the insteresting results of Chandra and XMM-Newton observatories is the discovery of sharp structures in the X-ray surface brightness of galaxy clusters. These structures (a.k.a. cold fronts) are likely associated with the contacted discontinuities formed when a hot gas flows over a colder gravitationally bound gas cloud. ...

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The new view on the population of Galactic open clusters A.E.Piskunov1, N.V.Kharchenko2, S.RЖser3, E.Schilbach3, R.-D.Scholz4 1 2 3 4 Institute of Astronomy, Moscow, Russia Main Astronomical ... Observatory, Kiev, Ukraine Astronomisches Rechen-Institut, Heidelberg, Germany Astrophysikalisches Institut Potsdam, Germany What are open clusters and what do they teach us Groups of Population I ... Cluster complexes: OCC-1 = Gould's Belt cluster complex? ...

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... Cepheids and star groupings Sternberg Institute, Moscow University, 1983 Professor, 1997 Employment: 2000 -present Main sciential fellow, Sternberg Astronomicl Institute (SAI) of Moscow State University 1989 - 2000 Head of the Department for Galactic and Variable Stars Researches, SAI 1986 - 1989: Leading Scientific Fellow, SAI 1973 - 1986: Senior Scientific Fellow, SAI 1960 - 1973: laborant, aspirant ... 22, 161, 1978 3) Star complexes. ... Astron. ... Large scale star formation in galaxies. ...

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• Yuri Nicolaevich Efremov - My Home Page
• Division of the Galaxy and Variable Stars
• Maidanak Lab page

... The study of the Large-scale structure of the Universe and measurements of the Dark Energy equation of state; The exploration of the growth and cosmological evolution of supermassive Black holes in the Universe. ... In course of the all sky survey SRG will discover about 100 000 galaxy clusters and 3 million AGNs. Galaxy clusters are the largest gravitationally bounded objects in the Universe and are best explored through the study of X-ray emission from the hot intergalactic gas. ... 2016 IKI RAN ...

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• Second Spectrum-RG/eROSITA Conference
• z90-program

... Dept. for Physics of Stars&Galaxies . ... Using a database view Sloan Digital Sky Survey (SDSS), containing almost a million spectra created 15,000 sample galaxies with active star formation, which is used for various studies and physical state of evolution of galaxies. ... Star clusters of the Galaxy . The project MWSC (Milky Way Star Clusters) directory using 2MASS, which includes nearly 500 million vision to the limit Ks = 15.3, analyzed more than 4,000 cluster-like objects in the galaxy. ...

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• MAO NASU :: Topic: 1st Announcement IAU Symposium 312 Star Clusters and Black
• The Laboratory of Astrometry
• Research - Page 2

... Today this year's largest group of sunspots will cross the Sun's central meridian. ... The next day, the number of spots in the group reached five, and the day after, on June 2nd, it was possible to count thirteen sunspots on solar disk, which had been clear prior to this. ... This year's two most powerful active areas, which passed across the solar disk at the beginning of May, 2009, are set to appear in the Sun's eastern sector in two days, on June 6th. ...

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... IAU planet classification Observing with a Telescope Large Scale Structure The observables: Local Group (size 1 Mpc) Virgo cluster (size 2+ Mpc) Virgo supercluster (size ~33 Mpc) Voids (size ~ 10-150 Mpc), Walls and sheets, aka filaments (size ~ 50-80+ Mpc) 1 parsec The nearest star is 1.2 parsecs away (Proxima Centuri). ... Virgo supercluster Voids, Sheets Filaments The Virgo Cluster is a cluster of galaxies at a distance of about 18.0 Mpc away in the constellation Virgo. ...

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• http://www.aaa.org/s932/images/09fallclass4.pdf

Feb 28 2016 Lacerta - The Lizard IC 1434 11mmT6 Open Cluster 12.0 III 2 m LOOSE GROUP,15-20 STARS,R=F Nov 16 2012 18 IC 1442 11mmT6 Open Cluster 12.0 III 1 p TIGHT GROUP, STARS=20+,R=F Nov 16 2012 18 IC 5180 7mm TV VF,PS,UB, NND ,AV1,R=F Galaxy E: Sep 14 2012 18 IC 5217 11mmT6 VS,VF,R=F Planetary Neb 2 Nov 16 2012 18 MAC 2221+3632 17mmT4 VF,ES,R, NND ,AV,R=F Galaxy Sep 11 ...

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• http://www.wro.org/neumann/RNGC_by_Constellation-Cep.pdf
• http://www.wro.org/neumann/RNGC_by_Constellation-Aql.pdf
• http://www.wro.org/neumann/RNGC_by_Constellation-Gem.pdf

... Ciel Espace, le magazine qui vous guide toujours plus loin . ... Ciel Espace, nouvelle formule, c'est . des actualit†йs . ... des pages consacr†йes †а la publication de vos photos Mais c'est aussi une vraie communaut†й avec laquelle partager votre passion et nourrir votre curiosit†й. Accueil Fusion de galaxies naines †а proximit†й de la Voie lact†йe . ... 07/04/2016 - Plong†йe au centre de la Voie lact†йe . ... 25/02/2016 - La Voie lact†йe cartographi†йe en ondes millim†йtriques . ...

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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 в 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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... All previous such superstars have been found along with many companion stars in the centres of crowded star clusters. The star is known as VFTS 682 from the VLT-FLAMES Tarantula Survey catalogue of the European Southern Observatory's Very Large Telescope (VLT) located at Paranal in Chile by means of the attached FLAMES instrument. ... Although VFTS 682 seems to be alone now it is not very far away from a very rich star cluster known as RMC 136 that contains several similar superstars. ...

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• William Herschel
• Astronomy Today and the Role Played by the Hubble Space Telescope: Wednesday 17
• Armagh Observatory Press Release

Эта одна из наиболее близких групп галактик (среднее расстояние до группы около 3.5 Мпк), но по структуре она совершенно отличается от Местной Группы (МГ). По видимому и эволюция галактик в этой группе проходила по другому. По числу членов группа M81 богаче МГ раза в два. К этой группе принадлежит довольно много интересных объектов. ... Галактики группы M81/NGC2403 . ... 3.6 . ... N3031,M81 . ... cirr? ... The Local Group in comparison with other nearby groups of galaxies' . ...

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• The M101 group of galaxies
• The Sculptor group of galaxies
• Vladimir P. Reshetnikov's Home Page

... The search for distant objects which can be both galaxies and quasars is one of the most important problems of observational astrphysics, because it allows one to determine cosmological parameters connected with the time of appearence and evolution of stellar systems, large scale structure of the Universe. ... Radio galaxies are important objects to be studied because they are sources of infrared-optical-ultraviolet continuum, emission lines and continual radio emission. ...

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• Апробация результатов
• Publications
• About laboratory

... Thursday August 13 . Friday August 14 . ... 11.00 12.15 . ... Maxim NAZAROV : Yangians and classical Lie algebras . One of the discoveries of G. I. Olshanski is the link between the classical Lie algebras and affine quantum groups, namely Yangians. ... Yuri NERETIN : Double coset multiplication on infinite-dimensional classical groups . ... The meeting will take place in Moscow, on August 13 14, 2009, at the premises of the A. A. Kharkevich Institute for Information Transmission Problems . ...

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• Registration Form
• Transformation Groups 2007
• Laminations and group actions in€аdynamics

THE SUBSYSTEMS OF THE MILKY WAY HALO. ... A catalogue of homogeneous fundamental astrophysical parameters for 145 globular clusters is composed on the base of the data of compilative catalogue by Harris (1997) and from another literature. ... In addition, it has large rotation velocity ( V rot =77?33 km/s), appreciable radial and vertical metallicity gradients equal by value, and has the oldest average age (subsystem of the old halo). ... Characteristic parameter of globular cluster subsystems. ...

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• Vladimir Marsakov Abstracts
• T.Borkova, V.Marsakov, Subsystems of the Galactic halo, their structures and
• T.Borkova, V.Marsakov, Distant globular clusters with anomalously small masses

... Session 1 - Stars, star formation, stellar populations and planets . 9.20 10.00 . ... HST Spectroscopy of the Hottest White Dwarfs . ... Coffee break . ... Lunch break . ... A (long) look at neutron stars with HST . ... Session 2 - Nearby galaxies, bulges, spheroids, galaxy formation . ... New HST/ACS Insights into the Evolution of Star-Forming Dwarf Galaxies with Extreme Properties of Cosmological Relevance . ... Deriving properties of Lyman-break galaxies at z~3-5 using HST/VLT/Spitzer data . ...

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• ESA-ESO Working Groups
• ESA/ESO Working Groups
• The Formation and Evolution of LMC Rich Star Clusters: NGC 1818

... 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/my_an.pdf
• http://sn.sai.msu.ru/~sil/preprints/mykukar.pdf

... Parent Directory 05-Aug-2008 17:34 - 66ophN_1.eps 15-Apr-2008 13:18 187k 66ophN_2.eps 15-Apr-2008 13:18 188k 66ophN_3.eps 15-Apr-2008 13:18 193k 66ophN_4.eps 15-Apr-2008 13:18 182k 66ophN_5.eps 15-Apr-2008 13:18 147k 66ophS_art_1.eps 10-Jun-2009 05:08 91k 66ophS_art_2.eps 10-Jun-2009 05:08 97k 66ophS_art_3.eps 10-Jun-2009 05:08 97k 66ophS_art_4.eps 10-Jun-2009 05:09 100k 66ophS_art_5.eps 10-Jun-2009 05:09 102k 66ophS_art_6.eps ...

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• Index of /groups/cluster/gcvs/digit
• Index of /groups/cluster/gcvs/digit/preprint.files
• Index of /groups/cluster/gcvs/gcvs/nl