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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• Low Surface Brightness Galaxy Gallery
• Astronomy Plus CCD Images of Galaxies
• Galaxy Gallery Page II

Welcome to the Starburst and Galaxy Evolution website.

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• Metallicity Effects on Dust Properties in Starbursting Galaxies
• Dust Attenuation in Late-Type Galaxies. I. Effects on Bulge and Disk Components
• Attenuation Effects in Spiral Galaxies: Multiwavelength Photometry and Disk

... Credit Copyright: Hubble Legacy Archive , ESA , NASA ; Processing - Martin Pugh Explanation: NGC 3314 is actually two large spiral galaxies which just happen to almost exactly line up. ... But against the glow of the background galaxy, dark swirling lanes of interstellar dust appear to dominate the face-on spiral's structure. ... Publications with keywords: NGC 3314 - spiral galaxy - dust - dust lanes . Publications with words: NGC 3314 - spiral galaxy - dust - dust lanes . ...

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• A Galaxy Gravitational Lens
• Астронет > A Galaxy Gravitational Lens
• Galaxy, Stars, and Dust

... In this talk, I will discuss a study of the effect of ionization on the low end of HI mass function. The existence of a large population of low mass galaxies follows from CDM theory. ... HIDEEP found no low HI column density galaxies. One possible explanation is that the disks are "frozen". ... We assume that galaxies are exposed to an ionizing background radiation, from a uniform quasar distribution. ... We find a gap in the average column densities around N H which drops to 10 17 cm -2 . ...

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• The Dark Side of the Galaxy: a Skiagraphic Panorama of Cold H I
• REU Science Area
• Cold Atomic Hydrogen in the Galaxy

... 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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... Primordial theory review : Dick Bond . Defects and the CMB review : Andy Albrecht . ... Gravitational wave contribution to CMB anisotropies : V.B. Lukash and E.V. Mikheeva . C_l from cosmic strings : Lloyd Knox . Some aspects of CMB anisotropies induced from topological defects : Mairi Sakellariadou . ... CMB anisotropies from scaling sources : Ruth Durrer . ... SZ observations I : Sarah Church . ... Holes in the microwave sky? ... Detecting cosmic strings in the CMB : James Robinson . ...

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• Astrophysics Group Cosmic Microwave Background (CMB)
• Galaxy Evolution: Radio sources and their environments
• Astrophysics Group Cosmology

... December 20, 1995 . A Galaxy Gravitational Lens . Credit: NASA , HST , K. Ratnatunga. ... Around the center of the red galaxy image in the above photograph lie four blue "smudges." Each smudge is actually a different image of the same background quasar . ... Consequently, the huge mass of the galaxy is able to pull separate images of the quasar around it - an effect called gravitational lensing . Hence we see a gravitational mirage! ... About APOD | ... NASA Technical Rep.: ...

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• APOD: 2011 July 15 - NGC 3314: When Galaxies Overlap
• APOD: 2009 September 21 - Abell 370: Galaxy Cluster Gravitational Lens
• APOD: December 23, 1998 - Ring Around the Galaxy

An Ancient Universe: How Astronomers Know the Vast Scale of Cosmic Time . THE ANCIENT UNIVERSE . c) The Age of Light from the Most Distant Galaxies: The "Time Machine" Effect . ... Thus we are actually seeing these galaxies not as they are today, but as they were billions of years ago. ... The Universe: An Overview | ... The Ancient Universe - The Age of the Expanding Universe - The Age of the Oldest Stars - The Age of Light From Distant Galaxies - The Age of the Chemical Elements | ...

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• ASP: Good Astronomy Activities on the WWW
• ASP: Beacons in the Gloom
• ASP: An Ancient Universe - Changes in the Universe

Astronotes Armagh Planetarium's Stellar Blog! ... Stars . ... Starbursts are short-lived events, stars are forming so quickly that the reservoirs of interstellar gas from which stars are coalescing would be used up on a timescale much shorter than the age of the galaxy . ... Strong stellar winds from giant new stars in the starburst region combine with the blasts of supernovae to push a mighty flood of extremely hot gas, a ?superwind? from the galaxy thousands of light years into intergalactic space. ...

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• Expanding Universe | Astronotes
• ESO finds weird doomed planet from another galaxy | Astronotes
• Other Galaxies | Astronotes

This animation shows a galaxy cluster with two mass concentrations (the pink shading indicates the projected mass density) lensing a background field of faint blue galaxies. ... Inside the Einstein ring radius one has radial arcs, and right in the center of the cluster there are demagnified images. The highest magnifications occur at the Einstein ring radius, giving the large tangential arcs. ... Abell 2218 and CL2244-02 are clusters with tangential arcs. ... Tutorial : Part 1 | Part 2 | ...

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• Documentation: LEDA: parameter: bar
• "Structure" publications for 1997 year
• Cosmic InfraRed Background Radiation

... 1997: . The character of internal motions of gas in 7200 HI clouds in the outer region of our Galaxy was investigated according to the data of the HI survey with the RATAN-600. It turned out that the effect of turbulence, as the main mechanism of gas motion is not essential, while it was discovered that 36% of the clouds are rotating. ... Periodic variations of optical emission of the gamma, X-ray and radio pulsar GEMINGA were for the first time discovered from the observations with the BTA. ...

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• Galaxy sector, archive 2014
• RCJ0311+0507
• Galaxy sector, archive 1998

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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• Gravitational wave background from nearby galaxies
• A Gravitational Wave Map of Nearby Galaxies
• Amplitude Distribution

... Galaxies 99 Cosmic background with model of cloudy interstellar medium Yu. ... Figure 1: Averaged spectrum of the cosmic background I f in frequency range 0.25 200 MHz for the Galactic poles. ... First interpretation of the cosmic noise background spectrum at broad band frequency range 0.25 200 MHz with a model of the cloudy interstellar medium ISM is presented here. ... Synthesized background spectra I f for regions of the Galactic poles at the frequency range 0.25 200 MHz is presented in Fig. ...

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... 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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• Stars and Galaxies
• Is merging important for the size and mass growth of galaxies?
• Colours and magnitudes

... radiative transfer studies in the dawn . ... Background: The interstellar medium of spiral galaxies is filled by gas and small solid particles, dust grains. ... dust emission at longer wavelengths, as FIR or the submm (bottom picture) allows a direct detection of the grains. ... An ESF workshop on dust in spiral galaxies : European astronomers have always been at the forefront of FIR astronomy, the study of interstellar dust and the development of radiative transfer codes. ...

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• Clumpy dust disks
• Atlas of Monte Carlo Models of Dust Extinction in Galaxies
• Dust in Spiral Galaxies

... 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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• Cosmological Gene project
• Fabry-Perot Interferometer: Gallery Old
• GRB follow-up team

... Your main research interests concern neutral hydrogen. ... That means that there must be enormous quantities of gas lying around, waiting for the chance to collapse under its own weight into lumps and form stars and galaxies. If we could actually observe this gas, as it moves around and assembles itself into lumps, we would be directly observing the process of galaxy formation. ... Optical astronomers seem to think that they can observe galaxy formation by taking optical images. ... In galaxies. ...

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• VV29 = Arp 188 = The Chainsaw Galaxy
• David Nicholls: CV and publications
• CHIAKI's Research

... Astronomy news . ... NASA's Spitzer Images Out-of-This-World Galaxy . ... It is spiral-shaped like our Milky Way, with long, spindly arms of stars. The "eye" at the center of the galaxy is actually a monstrous black hole surrounded by a ring of stars. In this color-coded infrared view from Spitzer, the area around the invisible black hole is blue and the ring of stars, white. ... The ring around the black hole is bursting with new star formation. ...

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1st of August 2015 . Radio Galaxy Zoo: host galaxies and radio morphologies derived from visual inspection . ... We present results from the first twelve months of operation of Radio Galaxy Zoo 75% consensus among the Radio Galaxy Zoo cross-identifications, the project participants are as effective as the science experts at identifying the host galaxies. ... 2015, MNRAS, accepted . ... today * ATNF | ...

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• A new twist to polar rings
• The Circinus Galaxy
• Evolutionary Paths in Galaxy Morphology