... 18 Sep 19 1984 12.5" 16mm Jul 30 1981 12.5" 16mm MF,ML,ELONG-REC SHAPE,MANY *'S APPROX SAME MAG,MANY *'S RESOLVED ELONG,*'S 10.. ... 9 MAG,MB,ML EASILY DET NGC 6842 Planetary Neb 3b F,PL,VLE Jun 27 2003 12.5 9mmT6 Jul 30 1981 12.5 12mm MB,ML,PATCHY AREAS DET,R,SHISB WITH OIII FILTER,R=E VDIF,LOC IN SOMEWHAT BARREN * FIELD,VF,MS,F*'S INSIDE OF GLOW,NOT SURE OF DET NGC 6853 M27 Planetary Neb 3+2 VB,VL,BIN,IE,DUMBBEL 17mmT4 Jul 05 2008 31 Mar 22 2004 12.5 12mmT4 Aug 20 ...

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• http://www.wro.org/neumann/RNGC_by_Constellation-Cep.pdf
• http://www.wro.org/neumann/RNGC_by_Constellation-Pup.pdf
• http://www.wro.org/scodova/RNGC_by_Constellation-Sct.pdf

... Galaxy clusters in presence of dark energy: a kinetic approach . ... The external regions of galaxy clusters may be under strong influence of the dark energy, which was discovered by observations of supernovae Ia at redshift z < 1. The presence of the dark energy in the gravitational equilibrium equation, with the Einstein ? ... diagram where equilibrium solutions are not possible. ... Galactic Cluster in the Presence of Dark Energy . ...

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• http://www.cosmos.ru/vprokhor/multisat/200010/cg.cng
• http://www.cosmos.ru/vprokhor/multisat/200010/cp.cng
• http://www.iki.rssi.ru/comp/2013/gilfanov1_annotation.htm

... 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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• Deep Sky Images by Joe DiNapoli ? Amateur Astronomers Association of New York

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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... 320, P L45-L48 (1997). Abstract . ... 320, P L49-L52 (1997). ... 320, P L53-L56 (1997). ... 320, P L57-L59 (1997). ... 320, P 685-695 (1997). ... 320, P 696-704 (1997). ... 320, P 705-716 (1997). ... 320, P 717-730 (1997). ... 320, P 731-745 (1997). ... 320, P 746-756 (1997). ... 320, P 757-775 (1997). ... 320, P 776-782 (1997). ... 320, P 783-786 (1997). ... 320, P 787-790 (1997). ... 320, P 791-798 (1997). ... 320, P 799-810 (1997). ... 320, P 811-822 (1997). ... helpdesk@link.springer.de . ...

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• Springer LINK:A&A-EE: Table of Contents Volume 317 Number 3 (1997)
• Springer LINK:A&A-EE: Table of Contents Volume 323 Number 2 (1997)
• Springer LINK:A&A-EE: Table of Contents Volume 320 Number 1 (1997)

... Subject and Problems of Stellar Astronomy. ... Plane of Galaxy, Methods of Its Location Determination. ... Stars Distances. ... Other Methods of Stars Distances Determination. ... Tangential Velocities, Their Determination by Self-Motions. ... Determination of Solar Apex and Spatial Velocity by Radial and Spatial Velocities of Stars. ... Features of Orientation and Parameters of Peculiar Stellar Velocities Ellipsoid. ... General and Selective Light Absorption in Galaxy. ... Darc Clouds in Galaxy. ...

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• Extragalactic Astronomy

... Cluster Antares . ... Dual Intel Xeon 2.4 GHz, RAM 4GB, HDD 36GB + 73 GB RAID 0 массив . Сервер приложений (Linux) - IBM Intel Xeon 2.8 GHz, RAM 4 GB . Сервер приложений(Windows 2003 Server) - IBM Intel Xeon 3.2 GHz, RAM 4 GB . ... Dual dedicated connectivity: 100MBit/s + 1GBit/s. PVM 3.4.6, Atlas, MPI (MPICH2), HPL, PGI CDK (HPF) . GPU сервер "Tesla" : AMD Phenom (4 cores) + Nvidia Tesla C1060 GPU . ... Intel C++ compiler . ... Intel Cluster Toolkit Compiler Edition for Linux 3.2 . ...

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... In the past used to check pn/ MOS cross calibration Example of old vs new pn/ mos Residuals in the form of ratio data / model for PN data on MOS best fitting model Example of old vs new pn/ mos Residuals in the form of ratio data / model for PN data on MOS best fitting model ACIS S3 vs EPIC pn Ї Ї Same thing, only now we compare Chandra ACIS S3 with ... Flux cross-cal Ї Ї The new HRMA calibration impacts on the ACIS/EPIC flux cross calibration. ...

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• http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/presentations/cal_standards_collection.pdf
• scisimngc2516

... Participants . ... At the same time, the combinatorial description of moduli spaces of Riemann surfaces and related quantization topics together with the related issues in cluster algebras continue to thrive, including generalizations to algebras of higher rank and investigating the related algebraic structures. ... The workshop will take place at three locations: the Independent University of Moscow (3 days), the Steklov Mathematical Institute (2 days) and the Higher School of Economics (1 day). ...

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• Conference Zeta functions

Central Bodies Masses of Selected Globular Clusters N.A.Shakht, A.A.Kiselev, Yu.N.Gnedin and E.A.Grosheva. The Main Astronomical (Pulkovo) Observatory RAS 47 Tuc ґNGC 104 RA 00 24 .1 Dec -72° 04 .9 Size = 30.9 mvis + 4. 0 m D from = 12,1 kpc, h m Cen - NGC 5139 NGC 6397 (Ara) RA 17 h40.m7 Dec -53o 40'.4 Size = 31',0 mvis + 5,3m D from =2.3 kpc RA 13h 26m .8 Dec -47° 28 6 Size = 36.3 m vis +3. 7 m D from =15.8 ?1.1 kpc, 12109 years, Age: 10109 years, (13.4 ? 0.8)109 years. ...

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• http://www.puldb.ru/jenam_2011/PUB_JENAM_2011/shakht_2.pdf
• http://www.puldb.ru/jenam_2011/jenam_present.pdf

В магнитосфере Земли обнаружены микровихри . 17 августа 2005 г . В 2000 г. Европейское космическое агентство отправило на околоземную орбиту квартет одинаковых спутников Cluster (все они имеют танцевальные названия - Salsa, Samba, Tango и Rumba). ... Тогда четверка спутников располагалась на орбите по углам воображаемого правильного тетраэдра, все стороны которого имели длину 100 км. ... Предыдущий документ - Следующий документ . ... Планета Земля . ...

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• В поле Земли обнаружена воронка
• Головная ударная волна обнаружена в магнитосфере Земли

This page is devoted to information on Supernova 1999gi in NGC 3184 . ... Information on the original web pages for many of these images can be found on the Supernova links web page. ... NGC 3184 is a fairly close Mag 10.3 galaxy, only about half as distant as the Virgo cluster. ... Seiichi Yoshida has a 1999gi page . Odd Trondal's 1999gi page . ... CfA image . ... 14.5 . ... Jean Marie Llapasset image . ... vsnet-alert 3805 ] SN 1999gi in NGC 3184 . vsnet-chat 2438 ] Host galaxy of SN1999gi . ...

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• Supernova 2002bu in NGC 4242
• Supernova 1994D in NGC 4526
• Supernova 1999cf in UGC 8539

... 2001 - present-day Researcher in Theoretical Department of Astro Space Center of Lebedev Physical Institute ot RAS . ... Department Number . ... Astro Space Center . ... arna@lukash.asc.rssi.ru . ... Arkhipova N.A., Komberg B.V., Lukash V.N., Mikheeva E.V., "Population of Cosmic Voids", Astronomy Reports 51, pp 787-796 (2007) . ... Surdin, V.G., Arkhipova, N.A., "Influence of dissipation and dynamical friction on the number of globular clusters in a galaxy", Astronomy Letters, Vol.24, p.343 (1998) ...

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• Beloborodov Andrei Mikhailovich, Astro Space Center (ASC)
• ASC site, Russian version

... STELLAR DYNAMICS: FROM CLASSIC TO MODERN . ... Sobolev Astronomical Institute, Saint Petersburg State University, Russia . ... The proposed meeting is being organized by the St.Petersburg State University, assisted by an international Scientific Organizing Committee, and marks the centennial of Professor K.F.Ogorodnikov's birth. ... The conference will be organized by the Sobolev Astronomical Institute of St.Petersburg State University in the building of the Faculty of Mathematics and Mechanics. ...

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ARCSAT ID NUMBER: AS05 DESCRIPTIVE TITLE: Fundamental Properties of High Galactic Latitude Open Clusters PI: Ana Larson OBSERVER(S): Ana Larson, Joanne Hughes Clark UNCERTIFIED/UNTRAINED OBSERVERS:Daniel Larsen, Max Lutz COLLABORATORS: Joanne Hughes Clark CONTACT INFORMATION: dlarsen9@uw.edu 808-987-2176 lutzm@uw.edu 425-749-2812 jhughes@seattleu.edu anamunn@uw.edu TIME REQUESTED: ...

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• http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_oct2015/AS06.html
• http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_oct2014/AS06.html
• http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_may2014/AS10.html

... AstroGuide | ... Astro Images . ... M45, Pleiades Cluster . Image by John Chumack, Galactic Images . M45 The Pleiades Cluster "The Seven Sisters." 45 minute exposure through 6: Takahashi Astrograph. Courtesy of John Chumack, Galactic Images . ... www.astronomy.net . About Astronomy Net | ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . are trademarks of John Huggins ...

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• What I See - an Astronomy Net Observation_reports Forum Message
• The Astronomy Shop - Books - by Astronomy Net
• The Astronomy Shop - Calendars - by Astronomy Net

... Laboratory of Real Structure of Crystals . ... Fields of research . Experimental techniques . ... Photoelasticity method for study of microstress fields around individual dislocations (and their clusters) and their influence on physical properties of crystals. ... Two-level periodic pulse loading technique for study of characteristics of the kink pair formation and motion along dislocation lines in different types of crystals. ISSP RAS ? 2006 All rights reserved ...

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• Phys. Rev. B 54, 454 (1996): Neminsky et al. - ac susceptibility of Rb
• SNL ISSP RAS
• Seminars

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

ASTEROIDAL DAMAGE TO THE EARTH: IMPLICATIONS BY ASTEROIDS ґ RUBBLE PILES. ... 13, Moscow 119892, Russia, E-mail:san@sai.msu.ru In the cause of asteroids ґ rubble piles its effective cross-section of collision to the Earth is determined not by consolidated body, but by cluster of its fragments. Since the stage of rubble ґ piles may be ~108 years (see our communication at previous symposium), it may be significant for estimation the asteroidal damage to the Earth. ...

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• http://selena.sai.msu.ru/San/Publications/ms42/m42_46.pdf

... Сроки проведения: July 4-6, 2005 . Место проведения: Rome, Italy . Deadline for submission of application: February 15, 2005 . Web-Information: http://newyork.ing.uniroma1.it/neuwb2/ . ... Сроки проведения: 25-28 сентября 2005 г. Место проведения: Суздаль, Россия . ... Сроки проведения: 12-16 сентября 2005 г. Место проведения: Севастополь, Крым, Украина . Срок представления докладов: 11 мая 2005 г. Web-Information: http://ieee.orbita.ru/aps/crim05r.htm . ...

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