Next: Sunday pm #1 Up: Minutes of the 1st Previous: HVCs . ... Blitz et al. (1999) and Braun Burton (1999) have suggested that some HVCs have median distances of 500 kpc to 1 Mpc and HI masses of 10 6 - 7 solar masses. ... Simulations of galaxy formation, e.g. Klypin et al. (1999), predict large numbers of satellites in Local Group analogs. ... Detections were identified by searching by eye cuts through the cubes. ... Consider a comparison of the Parkes Multibeam with ALFA: . ... Parkes MB . ...

We present H I imaging of the galaxy group IC 1459 carried out with six antennas of the Australian Square Kilometre Array Pathfinder equipped with phased-array feeds. ... We present H I images, velocity fields and integrated spectra of all detections, and highlight the discovery of three H I clouds - two in the proximity of the galaxy IC 5270 and one close to NGC 7418. Each cloud has an H I mass of ~109 Msun and accounts for ~15 per cent of the H I associated with its host galaxy. ...

This home page belongs to small group of scientists working at . Sternberg Astronomical Institute which is a part of Moscow State University . ... Электронная библиотека научно-технической и художественной литературы (доступна только из ГАИШ) . ... Local staff . Dr. Edward Kononovich (konon -at- sai.msu.ru), Associate Professor . ... Dr. Sergey Ayukov (asv -at- sai.msu.ru), Research Fellow, Webmaster of the group . ... Joint seminar of Solar Studies Structure Group and Solar Photometry Group . ...

Sternberg Astronomical Institute, Moscow University, . Moscow, Russia . Supernovae make us brighter .. Search russian astronomical resources . Mirror of International Supernovae Network ( Original site ) . Catalogue of Supernovae Stars . HTTP access to SAI Catalogue of Supernovae Stars . SAI SN Light Curves Online . ... Sternberg Astronomical Institute ( in Russian ) . ... Astronet - Russian Astronomical Network . ... Russian Foundation for Basic Research . ...

... Credit Copyright: Nicolюs Villegas Explanation: Large galaxies and faint nebulae highlight this deep image of the M81 Group of galaxies. ... Around the image many other galaxies from the M81 Group of galaxies can be seen, as well as a lucky satellite glint streaking across the image left. ... This whole galaxy menagerie is seen through the faint glow of an Integrated Flux Nebula , a little studied complex of diffuse gas and dust clouds in our Milky Way Galaxy . ... Galaxy Wars: M81 versus M82 . ...

... Laboratory "Structure" was created in 1992 from the temporary scientific group formed in 1988 in SAO RAS. In December 2003 it was transformed into group of Physics and Evolution of Galaxies , which enters into new Laboratory of Extragalactic ASTROPHYSICS and COSMOLOGY. ... Kniazev A.Y. senior researcher, associated foreign member . Kniazeva T.F. junior researcher, associated foreign member . ... Lipovetsky Valentin A. (1945-1996) former leader of the Laboratory . ...

... Access key help . ... Astrophysics Group . ... Galaxy Formation and Evolution . Main Projects . ... PhD Thesis Projects . ... One of the main goals of the instrument is to identify and characterise the first galaxies formed in the early Universe and to track their evolution through the cosmic epoch by delivering the deepest spectra ever obtained for these objects in the near-IR range. ... SPIRE programme) on the evolution of the dust content in galaxies. ...

... HST . ... Data . ... Hubble Heritage Project . ... HST Overview . ... Cycle 24 Announcement . ... Retrieving HST Data . ... 03/16/2004 - The ACS-WFC raw data and the associated calibration files for the Hubble Ultra Deep Field are now available. ... Also, a nice Javascript viewer for browsing the UDF field is now available. ... The ACS Ultra Deep Field (UDF) is a survey carried out using the Advanced Camera for Surveys ( ACS ) on HST and taking advantage of the Director's Discretionary time. ...

... Next: Cheating Poisson: A Up: Statistical Analysis Previous: Spatial Models and . ... The spatial distribution of stars in the Local Group dwarf irregular galaxy NGC 6822 has been studied, using recent positions and deep photometry for about 15,000 stars in the galaxy. Based on photometrical data, OB stars and red stars could be studied separately. Spatial statistical tools have been applied to the analysis of the spatial structure. ... Figure: Model selection by the aid of CAIC . ...

... Our recent observations with the Hubble Space Telescope (August 29, 2014) led to revealing a highly isolated dwarf spheroidal galaxy KKs 3 situated at a distance of 2.12 0.07 Mpc from the Milky Way. The dSph galaxy locates on the southern sky (RA=02 h 24 m 44.4 s , Dec.= ... Over the last decade, about 30 dSph galaxies have been discovered inside the Local Group through systematic search in the vicinity of M31 and more that a dozen dSphs were discovered in the nearby group around M81. ...

... Home Gallery Astrophotography Deep Sky Images by Joe DiNapoli . ... Deep Sky Images by Joe DiNapoli . ... Deep Sky Gallery by Ed Fox . ... Beyond New York City . ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . Observing Resources for Amateur Astronomers - Part 2: Intermediate Observers . ... A History of the First Forty Years of the Amateur Astronomers Association . ... 2016 Amateur Astronomers Association of New York Designed by Press Customizr Powered by . ...

... History . ... The group for study of galaxies and cosmology has been created in April, 2011 and unified researchers from the laboratory of radio astrophysics (O.V.Verkhodanov, N.N.Bursov, N.V.Verkhodanova), the laboratory of antenna measurements (E.K.Maiorova) and researches from the radio astronomical sector (Yu.N.Parijskij, T.A.Semenova, V.A.Stolyarov) inside the laboratory of radio astrophysics by the order of the director of SAO according to the decision of the SAO Scientific coincil. ...

Research Area: Observational Astrophysics . Research Interests include: Galaxy Evolution , Large Scale Structure, CCD Sky Surveys. ... Research Area: Astrophysics . Research Interests include: accretion disks; dense fluids . ... Research Area : Experimental Astrophysics . Research Interests : Galaxy surveys, evolution and properties of galaxies, . Research Area: Theoretical Astrophysics . Research Interests include: Gravitational Wave formation, propagation and detection; . ...

. Main Sections LabIR main page . Instrument page . Documentation . Science Publications . Special Sections Software Page . Inside the Lab . LabIR staff . Companion Pages Skysoft Home . Tirgo Page . Tirgo Archive . LabIR Hotlist . Lunar occultations . AO star finder . Simple calculator .

... Tonight's Sky . ... The Magazine . News . Observing . ... Community . ... Gravitational wave search provides insights into galaxy evolution and mergers . ... The double star 54 Leonis, spiral galaxy NGC 3198, and emission nebula NGC 3199 . ... Open cluster NGC 2818, spiral galaxy NGC 2964, and spiral galaxy NGC 2976 . ... Astronomy for Kids . ... Local Group . ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ... Astronomy Magazine . ...

... Chandra Observation of DEEP2 Galaxy Groups and Clusters . ... Monday: 'Normal' Galaxies, Tuesday: Cluster Formation and Evolution . ... Statistics of galaxy groups in ultradeep XMM surveys. ... What can multiwavelength observations tell about cluster/group formation as well as galaxy evolution? ... I will present results from a Chandra study of eight low-redshift clusters that has systematically measured the AGN fraction in clusters and describe their spatial, kinematic, and host galaxy...

. A1332-45 . CEN5 . CEN6 . DDO161 . ESO222-10 . ESO223-09 . ESO272-25 . ESO274-01 . ESO324-24 . ESO325-11 . ESO381-20 . ESO383-87 . ESO444-84 . IC4316 . NGC4945 . NGC5068 . NGC5102 . NGC5128 . NGC5206 . NGC5236 (M83) . NGC5237 . NGC5253 . NGC5264 . NGC5404 . SGC1259-1659 . SGC1424-4604 . UGCA365 .

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' . ...

... Bad Astronomy . ... Dwingeloo 1 is a galaxy that's very close, yet no one saw it until pretty recently. ... Dwingeloo 1 is not alone in the cosmos; it is part of a close group of several galaxies. ... The galaxy group containing Dwingeloo 1 (actually, the group is named after the brightest member, IC 342) probably formed at the same time as the Milky Way, from a truly enormous cloud of hydrogen. ... Two large ones, orbiting each other, can pass a bit of that orbital energy to a smaller galaxy. ...

. of Lomonosov Moscow State University, . Russia . GCVS Research Group . Catalogues of Variable Stars . Future Prospects of Variable-Star Catalogues . B.V. Kukarkin Centenary Conference: Variable Stars, the Galactic Halo and Galaxy formation (VS-Halo) . What's new . Recent publications . Digitization of Moscow Plate Archive . The "Peremennye Zvezdy" (Variable Stars) journal . Send questions and comments to Olga Durlevich .