... HCG 87: A Small Group of Galaxies . ... Indeed, the galaxies of HCG 87 are gravitationally stretching each other during their 100-million year orbits around a common center. ... HCG 87 is composed of a large edge-on spiral galaxy visible near the image center, an elliptical galaxy visible to its right, and a spiral galaxy visible near the top. The small spiral near the center might be far in the distance. ... Studying groups like HCG 87 allows insight into how all galaxies form and evolve . ...

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• XWare > APOD

... 2015 August 9 . HCG 87: A Small Group of Galaxies . ... Explanation: Sometimes galaxies form groups. ... Indeed, the galaxies of HCG 87 are gravitationally stretching each other during their 100-million year orbits around a common center. ... HCG 87 is composed of a large edge-on spiral galaxy visible near the image center, an elliptical galaxy visible to its right, and a spiral galaxy visible near the top. ... Studying groups like HCG 87 allows insight into how all galaxies form and evolve . ...

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• APOD Index - Galaxies: Local Group
• SAI SN RESEARCH GROUP
• APOD: September 6, 1999 - HCG 87: A Small Group of Galaxies

... Neutral hydrogen observations of the spiral galaxies NGC 6221 and NGC 6215 with the Australia Telescope Compact Array (ATCA) reveal a wide, two-stranded bridge of at least 3 x 10^8 Msun which can be traced between the two galaxies over a projected distance of 100 kpc. ... The color figure below shows the HI emission (blue) in the bridge velocity range overlaid onto an optical image. ... A tidal HI bridge is visible between NGC 6221 and its brightest neighbour, NGC 6215 (v_sys = 1555 km/s). ...

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• The HIPASS Bright Galaxy Catalog
• The Compact Galaxy Group NGC 6845
• Pulsar Group Main/Animations

... 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. ...

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• important_en
• Group for study of galaxies and cosmology, staff

In this gallery are many images of Low Surface Brightness Galaxies which have recently been discovered and analyzed. ... The central surface brightness of this galaxy is 24.28 . Malin 2 This galaxy is another huge disk galaxy with a scale length of 15 kpc and a redshift of 15000 km/a. The high surface brightness knot in one of its spiral arms actually has the same color, luminosity and H-alpha equivalent width as the entire Large Magellanic Cloud . ... Truly it is a Low Surface Brightness Galaxy. ...

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• The Galaxy Gallery Page 6: Comparative Morphology
• The Galaxy Gallery: Messier Objects
• Galaxy Gallery Page II

... Armagh Planetarium . ... Universe . ... 1 Comment In July 2015, we will finally have our long-awaited closeup views of the dwarf planet Pluto and its moons when NASA?s New Horizons probe flies past the tiny and distant [ ] . ... No Comments As everyone knows on Friday 20 March 2015, a total solar eclipse will occur across the far northern regions of Europe and the Arctic. ... Here you will find the latest news and views from the fascinating worlds of astronomy and space exploration. ...

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• WLM Galaxy: a Cosmic Living Fossil | Astronotes
• Exoplanet HAT-P-1b: weird, warm and fuzzy | Astronotes
• Rings Around an Asteroid | Astronotes

... The Magazine . ... Observing . ... Magazine . ... Star Atlas . ... An artificial comet holds secrets to Earths life . ... stars . ... Observing Podcasts . ... Astronomy for Kids . ... Observing springtime deep-sky objects with a large telescope . Springtime observing for small telescopes . ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ... Click here to receive a FREE e-Guide exclusively from Astronomy magazine. ... Astronomy Magazine . ...

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• Galaxy groupings | Astronomy.com
• Bright planets meet at dusk | Astronomy.com
• Groups | Astronomy.com

... Planet Ziggy seems to be located in the outer regions of an elliptical galaxy, or perhaps in a globular cluster orbiting such a galaxy. ... We have not been able to detect any spiral galaxies elsewhere in the sky. ... Iif they are too small for their gravity to achieve this. force holding the two objects together ­ strongly suggests that these objects are Page 1 The Milk Stain No milky-way is seen. ... We are calling it the Milk Stain. This could be an elliptical galaxy or a globular cluster. ...

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• http://www.mso.anu.edu.au/pfrancis/roleplay/ziggy/model_answer2.doc
• GSAOI Dwarf Galaxies Science Page
• Galaxies of the Centaurus A group (in alphabetic order)

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 . ...

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... Astrophysics Group . ... Galaxies and Quasars . ... All galaxies emit radio waves as well as light. ... Often, they shoot out two jets, magnetic fields and very fast electrons (see below). ... This explains why we often see one very bright jet ? ... Quasars, the most powerful sources, often show a prominent jet, strong radio galaxies like the one to the right more usually don?t. The most powerful of these radio sources can be detected at immense distances in the Universe ? ...

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• Astrophysics Group Main Projects
• CO in NGC 1530, aperture synthesis of a barred spiral
• Astrophysics Group Galaxy Formation and Evolution

... Increases in IR surface brightness appear to be affected by both increased radiation field strength and increased local gas density. Individual regions and the galaxy as a whole fall within the observed scatter of recent high-resolution studies of the radio-far-IR correlation in nearby spiral galaxies; this is likely the result of depleted radio and far-IR emission strengths in the ISM of this dwarf galaxy. ...

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• Dust and Atomic Gas in Dwarf Irregular Galaxies of the M81 Group: The SINGS and
• Research Groups
• Our group

... Bringing news from across the Universe to children all around the world . ... Many of you will recognise the object in this space photograph as a galaxy: a collection of billions of bright, shining stars, and cosmic gas and dust. In this day and age, almost everyone has seen a photograph of a galaxy, making it hard to believe that less than 100 years ago most of the world s top astronomers didn t believe they existed! ... Before then, the existence of galaxies was uncertain. ...

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• http://www.eso.org/public/news/eso1128/kids/
• http://www.eso.org/public/news/eso1120/kids/
• ESO - NGG

... August 7, 1998 . M65 Without Moth . ... Explanation: Messier 65 ( M65 ) is a bright spiral galaxy of stars only 35 million light-years away in the constellation Leo . ... The faint blue smudges along the spiral arms of M65 are large clusters of bright, newly formed stars within the distant galaxy while the bright individual stars are foreground objects in our own Milky Way galaxy . ... About APOD > . ...

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• APOD: 2000 October 23 - Dwarf Elliptical Galaxy NGC 205 in the Local Group
• Arcetri Extragalactic Group
• APOD: 2000 August 18 - X-Rays From Antennae Galaxies

Our publications in 2004 year Kniazev, Alexei Y.; Grebel, Eva K.; Pustilnik, Simon A.; Pramskij, Alexander G.; Kniazeva, Tamara F.; Prada, Francisco; Harbeck, Daniel . ... 704-727 (02/2004) . Kniazev, A. Y.; Grebel, E. K.; Pramskij, A. G.; Pustilnik, S. A. American Astronomical Society Meeting 204, #80.06 (05/2004) . Pustilnik, S.; Kniazev, A.; Pramskij, A.; Izotov, Y.; Foltz, C.; Brosch, N.; Martin, J.-M.; Ugryumov, A. Astronomy and Astrophysics, v.419, p.469-484 (05/2004) . ... 419.. ...

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• Nearby Galaxies Catalogue (NBG)
• SAO: group Physics and Evolution of Galaxies home page
• Documentation: LEDA: parameter: lgg

... 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. ...

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... 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. ...

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• Group for study of galaxies and cosmology, staff
• astro-ph authors/title/abstract search for 'galaxy environment' all years

Text of these problems is available also in other languages : . ... What can one see in the Moon's sky more often - the Sun or the Earth? ... There are about of 250 millions of stars in the elliptical galaxy M32 (a satellite of Andromeda galaxy). ... The masses of Capella's components. ... You are proposed to estimate the masses of Capella's components, using our observational data. ... A galaxy's mass. ... Estimate the mass of FGC 1908 and compare it to the mass of our galaxy. ...

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• V International Astronomy Olympiad, Problems to solve (in English)

The Seyfert-2 NGC 7674: . ... As part of a larger project to study Luminous and Ultra-Luminous IR Galaxies in both H I absorption and radio continuum at high resolution, NGC 7674 was observed using the VLBA, the phased VLA, and the 305-m Arecibo radio telescope. ... Figure 1 shows a moderate resolution continuum image of the innermost 1 kpc region of NGC 7674 at 1.38 GHz and 20 milliarcsecond (mas) resolution. ... No absorption is detected toward the components J, W, and SW. ...

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• The Search for HVCs in Other Galaxies
• Arecibo Galaxy Environment Survey (AGES)
• The Evolution of Galaxies Seen Through The Neutral Hydrogen Line The Evolution

... 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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• Un anneau de galaxies naines autour d'AndromГЕde | Ciel et Espace

... Our Sun is part of a huge wheel-shaped collection of stars. ... Astronomers have long suspected it was a very massive black hole, and that every galaxy had such a central mass, created early in the history of the universe. ... However, unless that object happens to be headed directly at the black hole (a relatively small target) it will just swing around and fly away again, like a comet making a pass at the Sun. The velocity acquired in falling towards the black hole also helps it escape. ...

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• The Profile Constellation Mission
• The Celestial Sphere--lesson plan #1a
• The Path of the Sun, the Ecliptic --lesson plan #3