M1 image More About M1 Nice Color Picture . ... M16 image More About M16 HST image . ... M31 image More About M31 Nice Color Picture . ... M42 image ; M43 image More About M42/43 Nice Color CCD Picture . M51 image More About M51 Color Image of M51 M51 Supernova . M57 image More About M57 Nice Color CCD Picture Very Deep M57 Image . ... M81 image More About M81 M81 Supernova Ultraviolet Image of M81 More about Ultraviolet Imaging . M82 image More About M82 M82 False Color M82 True Color . ...

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... Light from a Extra Solar Planet . ... Light emitted by a planet far beyond our Solar System has been identified for the first time. The planet, illustrated in the above drawing, had its light detected by comparing the brightness of only.. NGC 1316: After Galaxies Collide . ... How did this strange-looking galaxy form? ... The Galactic Center Radio Arc . ... The pixelated planet above is actually our own planet Earth seen in gamma rays - the most energetic form of light. ... A Tether in Space . ...

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• Galaxy Group HCG 87

An image of the grand design of spiral galaxy M100 obtained with NASA's Hubble Space Telescope resolves individual stars within the majestic spiral arms. ... Hubble has the ability to resolve individual stars in other galaxies and measure accurately the light from very faint stars. This makes space telescope invaluable for identifying a rare class of pulsating stars, called Cepheid Variable stars embedded within M100's spiral arms. ... 617) 495-7062 . Fax: (617) 495-7356 . ...

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• The AstroStat Slog host galaxy

... 2003 July 31 . Galaxy Group HCG 87 . ... The large edge-on spiral near picture center, the fuzzy elliptical galaxy immediately to its right, and the spiral near the top of the image are identified members of the group, while the small spiral galaxy in the middle is likely a more distant background galaxy. ... While not exactly locked in a group hug , the HCG 87 galaxies are interacting gravitationally, influencing their fellow group members' structure and evolution. ... About APOD | ...

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• APOD: 2005 July 16 - Galaxy Group HCG 87
• APOD Index - Galaxies: Clusters of Galaxies
• APOD: 2009 August 29 - NGC 7771 Galaxy Group

... Our Galaxy . ... Stars . ... Image credit: ESO, Acknowledgement: VST/Omegacam Local Group Survey) . First observed in 1909, the WLM galaxy is part of the Local Group, about 10 million light years (3.1 Mpc) across, this is the set of more than 35 galaxies which includes our own Milky Way. ... I compared this little galaxy to a living fossil because looking at it gives us an insight into a past era in the UniverseтАЩs history. ... Distances and metallicities for 17 Local Group galaxies? . ...

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• Baby stars of NGC 2841 | Astronotes
• NGC4666: Secrets of a Starburst Galaxy | Astronotes
• Galaxy NGC 6744: the Milky Way's Cosmic Twin? | Astronotes

... The sample of the Local Volume galaxies (distance smaller than 10 Mpc) gives a unique opportunity to study the properties of galaxies including the weakest objects: the absolute magnitude M B -10 and the virial mass M vir 10 9 M x263C;. ... Luminosity function of the Local Volume galaxies. ... The luminosity functions for galaxies are presented: red dashed line - from the 2dFGRS survey (Norberg et al. 2002); blue dash-dotted line - from the SDSS survey (Blanton et al. ...

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• Measurement of the dark halo shape in polar ring galaxies
• RCJ0311+0507
• Galaxy sector, archive 2005

... Science/Nature | Vast halo extends galaxy's size 4/1/08 10:56 PM 08 Jan 07 12:23 Science/Nature Go Vast halo extends galaxy's size By Paul Rincon Science reporter, BBC News, Seattle Astronomers have found an enormous halo of stars around the Andromeda galaxy. ... In fact, Andromeda's "suburbs" are so vast that they nearly overlap with those of our own Milky Way galaxy. ... Andromeda is a spiral galaxy similar to the Milky Way. ... Science/Nature ) 'Alien' stars invade Milky Way (26 Sep 03 | ...

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• BBC NEWS | Science/Nature | Vast halo extends galaxy's size
• Starburst and Galaxy evolution
• Gaps in the Cloud Cover? Comparing Extinction Measures in Spiral Disks

... Confirmation that a mysterious cloud of hydrogen in the Virgo Cluster is a dark galaxy has been published by a team of astronomers . New evidence from NASA's Hubble Space Telescope and the Westerbork Synthesis Radio Telescope in the Netherlands has been used to rule out all but one of the ideas put forward to explain the existence of VIRGOHI 21, an intergalactic gas cloud 50 million light-years from the Earth. ... Only Dark Matter can account for the existence of such a system. ...

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• REU Science Area
• stars and galaxies hall

... STScI-PRC01-04 HUBBLE'S ULTRAVIOLET VIEWS OF NEARBY GALAXIES YIELD CLUES TO EARLY UNIVERSE Astronomers are using these three NASA Hubble Space Telescope images to help tackle the question of why distant galaxies have such odd shapes, appearing markedly different from the typical elliptical and spiral galaxies seen in the nearby universe. ... Light from these galaxies travels great distances (billions of light-years) to reach Earth. ... These stars emit mostly ultraviolet light. ...

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• STScI- PRC99-10: Hubble's Infrared Galaxy Gallery
• APOD: May 25, 1998 - M83: A Barred Spiral Galaxy
• Cannibal Stars Cause Giant Explosions in Fornax Cluster Galaxy (ESO Press

... We have made observations of the Perseus cluster with the Westerbork Telescope at 610 MHz. ... Several newly detected sources are identified with cluster galaxies. ... No evidence is found for the existence of the previously reported ~ 65'x25' cluster halo, 3C 84B. Key words: radio galaxies - clusters - tailed radio sources buoyancy The Perseus Cluster of galaxies is one of the most fascinating systems accessible to extragalactic astronomers. ...

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• Optically detected galaxies with POSSI-E in the "zone of avoidance. I-V
• Arcsecond Positions of UGC Galaxies
• A0690 radio identifications

... Gravitational wave search provides insights into galaxy evolution and mergers . ... galaxies . ... Tour the Deep Sky . ... Scientists identified galaxies at 600 million light-years after the Big Bang in the Hubble Ultra Deep Field. Shouldnт??t this light have passed us long ago? Why is it just getting to us now? ... Scientists viewed galaxies that date to a time just 600 million years after the Big Bang. ... Get instant access to subscriber content on Astronomy.com! ...

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• What are typical star-to-star distances in globular clusters compared to
• Hubble images quintuple quasar | Astronomy.com
• Astronomers discover quasars acting as gravitational lenses | Astronomy.com

In autumn 1994, two groups of astronomers announced that they had discovered Cepheid variable stars in a distant cluster of galaxies. ... As the term suggests, variable stars change in brightness over time. ... Variable stars are an ideal way to get high-school students doing real science, with real data, from the real sky. ... a sky chart to find the stars . ... Students can use the nearby stars to estimate the magnitude of Delta. ... Locate the star Delta in Cepheus and estimate its brightness . ...

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• ASP: Book Review
• ASP: The Universe At Your Fingertips Activities TOC
• ASP: An Ancient Universe - The Age of the Expanding Universe

... О Далекой Галактике . ... Теперь в Далекой Галактике вы всегда можете увидеть свежие фотографии Солнца. ... Форум . Форум "Далекой Галактики" - прекрасное место для общения всех астрономов. ... Новости из космоса . ... Подписаться на новости Далекой Галактики Вы можете здесь: . ... Новости из Далекой Галактики - популярно об Астрономии . ... Если вы хотите выразить свое мнение о сайте "Далекая Галактика", или просто почитать мнения других посетителей - пожалуйста, заходите в Гостевую книгу . ...

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. Back to A.Zasov's homepage.

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... 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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• GRB follow-up team

... Research . ... A rare hybrid morphology radio galaxy . ... In this project we will be able to investigate the environmental effect on star formation and galaxy evolution in individual galaxies falling into the cluster through radio observations of active galactic nuclei (AGN). Current models of galaxy evolution regulate the star formation rates within the simulated galaxies by invoking radio-mode feedback from AGN. ... Julie.Banfield@anu.edu.au . ...

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• COALA - Computational Astrophysics Laboratory
• The High-Z SN Search Description
• THE AUSTRALIAN NATIONAL UNIVERSITY

... ATNF Home . ... About ATNF overview . News | ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Mopra radio telescope . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... Now, new Australia Telescope observations of the polar ring galaxy NGC 4650a suggest that the dark matter in this galaxy lies in a flattened distribution aligned with the polar ring. ...

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• HI in Dwarf Galaxies - A Two Day Workshop
• Science Rationale
• Previous HI observations of dSph galaxies

... The BM effect causes low-luminosity blazars (particularly BL Lacs) to be missed in surveys because the apparent luminosity of the non-thermal nuclear source does not exceed that of the host galaxy by a large factor. ... Browne (1995). ... In addition to these objects, a large fraction of the newly-identified BL Lacs in our sample (10 of 22; see Table 5) have been so classified only by virtue of our usage of the expanded March? et al. (1996) definition of the BL Lac class. ... 1996). ...

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• Comparing APEX and ALMA views of star-forming galaxies in the early Universe |
• The Thousand-Ruby Galaxy | ESO
• ESO - Thesis Topic: Testing galaxy formation in high density environments - the

Next: Critical Frequencies and Gravitational Previous: Extragalactic Gravitational Wave Background . The number of binaries per frequency decade per solid angle from a separate stellar system (galaxy or cluster of galaxies) is . ... For example, for the Andromeda galaxy M31 ( rad, ) one gets . ... If the angular size of the galaxy is less than the angular resolution of the detector, the critical frequency is independent of the angular resolution, . ...

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• Introduction
• Gravitational wave background from nearby galaxies
• Gravitational Waves from Coalescing Compact Binary Stars

... Miyauchi-Isobe, N., Nakajima, K., & Maehara, H. 2003, in ASP Conf. ... KUG is a catalog of ultraviolet-excess galaxies which have been detected on two- or three-color Kiso Schmidt plates. ... Figure 1: KUG survey areas. ... 2003). ... Figure 2 shows the KUG objects (red dots), and SDSS DR1 galaxies (blue dots) which are sampled in accordance with the magnitude and color ranges of KUGs. Figure 2: SDSS DR1 galaxies over KUG objects. ... Figure 3: SDSS DR1 galaxies over KUG objects in A0225 area. ...

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• The Co-Addition Technique Applied to Images of Galaxy Cores
• Integrating the HST Guide Star Catalog into the NASA/IPAC Extragalactic