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 . ...

Еще в разделе: (Показать все результаты (>368) - zebu.uoregon.edu/ )

• Low Surface Brightness Galaxy Gallery
• Astronomy Plus CCD Images of Galaxies
• Galaxy Gallery Page IV: The Movies

Our publications in 1997 year Izotov, Yu. I.; Thuan, T. X.; Lipovetsky, V. A. Dwarf Galaxies: Probes for Galaxy Formation and Evolution, Joint Discussion 2, 21 August 1997, Kyoto, Japan. Izotov, Yuri I.; Thuan, Trinh X.; Lipovetsky, Valentin A. Astrophysical Journal Supplement, 01 1997, v.108, p.1 . ... Pustil'nik, S. A.; Lipovetsky, V. A.; Izotov, Y. I.; Brinks, E.; Thuan, T. X.; Knyazev, A. Y.; Neizvestnyi, S. I.; Ugryumov, A. V. Pis'ma Astron. ... 74, August 1997, p. 536 . ...

Еще в разделе: (Показать все результаты (>1510) - www.sao.ru/ )

• "Structure" publications in 2008 year
• "Structure" publications in 2006 year
• "Structure" publications in 1996 year

... Research . ... The aim of this project is to study the nearest spiral galaxies in the nearby Sculptor Group in neutral hydrogen with the ATCA to search for high-velocity clouds (HVCs) and extra-planar gas in their environment. ... The Sculptor Group is the nearest galaxy group. ... Therefore, we have mapped a large area of almost $2^{\circ} \times 2^{\circ}$ around the two nearest large Sculptor Group galaxies, NGC 55 and NGC 300, with the ATCA in mosaicking mode. ...

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• Structure and Evolution of Galaxies
• WALLABY - the ASKAP HI All-Sky Survey
• The Circinus Galaxy

... 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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• Laboratory of spectroscopy and photometry of extragalactic objects : Vortex1
• Laboratory of spectroscopy and photometry of extragalactic objects : Vortex
• Fabry-Perot Interferometer: Gallery Old

Welcome to the Starburst and Galaxy Evolution website.

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• The Opacity of Spiral Galaxy Disks. VIII. Structure of the Cold ISM
• Posters
• The Herschel Exploitation of Local Galaxy Andromeda (HELGA). I. Global

... Galaxy Evolution home . ... Regulating the ISM and star formation . Cosmological evolution of star-forming galaxies . ... Local Information . ... In order to investigate the cosmological evolution of star-forming galaxies it is essential that we understand the physics which controls the evolution and regulation of star formation in the ISM. ... We use a combined observational and numerical approach to study interacting and merging galaxies in the local Universe. ...

Еще в разделе: (Показать все результаты (>1073) - www.mrao.cam.ac.uk/ )

• Astrophysics Group Galaxy Formation and Evolution
• PPT Slide
• Galaxy Evolution: The origin and evoltuion of radio sources

. My astronomical research interests center on galaxy structure and evolution. Current topics include: . Polar-ring and interacting galaxies (see also new catalogue ) . Galaxy warps: statistics, properties and origin . Spiral galaxies at z~1: radial and vertical structure of stellar disks, statistics of interactions . Surface photometry and kinematics, dynamical modeling . Observational cosmology . Joomla Counter since Sep 1997

Еще в разделе: (Показать все результаты (>250) - www.astro.spbu.ru/ )

• List of publications
• Polar-Ring Galaxies
• A Nature of Polar-Ring Candidate Galaxy ZGC 2315+03

Topics covered by the IAU Symp. ... Do all galaxies have stellar halos? ... Stellar tracers of the MW halo and nearby galaxies; the stellar population of star clusters and their contribution to the galaxy halos . ... NEW: Scientific program of the IAU Symposium 317 can be downloaded here . ... GLOBAL PROPERTIES OF STELLAR HALOS FROM THE MILKY WAY TO EXTERNAL GALAXIES . ... DISCRETE CONSTITUENTS OF STELLAR HALOS IN THE MILKY WAY AND IN EXTERNAL GALAXIES : PLANETARY NEBULAE and GLOBULAR CLUSTERS . ...

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• ESO - PhD Thesis Topics offered by ESO Faculty Members
• ESO - Deconstructing Galaxies
• Ultra-compact dwarf galaxies

... We consider the astrophysical evolution of the Galaxy over large time scales, from early stages (an age of ~10 8 yrs) to the end of traditional stellar evolution (~10 11 yrs). ... In the model considered, the basic stages of Galactic evolution are as follows. ... Essentially all other basic parameters of the Galaxy vary little. ... The final "stellar epoch" in the life of the Galaxy is completed ~10 13 yrs after its formation, when the evolution of the least massive stars comes to an end. ...

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• Gradients in Disk Galaxies

... Numerical simulations of cosmic structure formation and evolution are now suggesting that a galaxy-cosmic web connection might be the key ingredient for regulating galaxy evolution, including the morphological type, star formation history and gas content. ... This is why the most basic questions remain 50 years after the first attempts to detect intergalactic gas: Is the intergalactic medium driving star formation? ... Last updated:09:26:07 05-Mar-2015 . ...

Еще в разделе: (Показать все результаты (>6513) - www.arcetri.astro.it/ )

• The impact of Warm Dark Matter on the ages of galaxies
• A local window on galaxy formation with ALMA
• SECCO1: an "almost-dark" dwarf galaxy

Next: Transparency of the Stochastic Up: Model of the Galaxy Previous: Frequency distribution of galactic . ... The parameters of the model resulted from a numerical fitting of various data, such as the observed distribution of the young star population and neutral hydrogen, the density of population II stars in the vicinity of the Sun, the galactic rotation curve and the dynamics and distribution of globular clusters   and dwarf irregular satellites of the Galaxy. ...

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• Model of the Galaxy
• Frequency distribution of galactic binaries
• Conference Programm

. First page Back Continue Last page Overview Graphics .

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• Heiles Symposium Presentations
• The Evolution of Galaxies through the Neutral Hydrogen Window The Evolution of
• The SMUDGES Survey

... 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 . ...

Еще в разделе: (Показать все результаты (>2) - fargalaxy.al.ru/ )

. Back to A.Zasov's homepage.

Еще в разделе: (Показать все результаты (>3) - neptun.sai.msu.su/ )

... Visible Distribution of Galaxies. ... Features of Elliptical, Lens-Shaped, Spiral and Irregular Galaxies. Galaxies with Bar. ... Distribution of Surface Brightness of Surface and Spiral Galaxies. ... Color Characteristics of Galaxies. ... Methods of Galaxies' Mass Determination. ... Hidden Mass of Spiral Galaxies. ... Features of Dark Matter Distribution in E and SO Galaxies. ... The Whole Number of Galaxies and Their Density by the Results of Observation on the 'Hubble' Space Telescope. ...

Еще в разделе: (Показать все результаты (>66) - space.univ.kiev.ua/ )

• Stellar Astronomy

... Credit: W. Schaap ( U. Gorningen ) et al., 2dF Galaxy Redshift Survey Explanation: What is the largest structure known? ... A grouping of galaxies known as the Sloan Great Wall was discovered in the Sloan Digital Sky Survey and is a leading candidate. The Sloan Great Wall can be seen in this digitally recast contour map of galaxies in the Two Degree Field galaxy survey. ... The labeled Sloan Great Wall spans over one billion light years, longer than any structure ever measured. ...

Еще в разделе: (Показать все результаты (>107251) - www.astronet.ru/ )

• Sextans A: A Seemingly Square Galaxy
• NGC 4651: The Umbrella Galaxy
• Астронет > Sextans A: A Seemingly Square Galaxy

... The formation of the disks of disk galaxies remains poorly understood. ... Many disk galaxies have only the thin disk component, with no bulge or significant thick disk. ... Almost all disk galaxies have an exponential radial surface brightness distribution. The reason for this exponential form is not known; nor is it known when the exponential form is established. ... We would compare low redshift galaxies observed in the I band with galaxies at z =0.5 in the J band and at z =1 in the H band. ...

Еще в разделе: (Показать все результаты (>558) - www.mso.anu.edu.au/ )

• Comparison of simulations with the large scale radio galaxy M87.
• Julie Banfield | Astronomer
• COALA - Computational Astrophysics Laboratory

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 . ...

Еще в разделе: (Показать все результаты (>744) - crydee.sai.msu.ru/ )

• ApSA courses
• Springer LINK:A&A-EE: Table of Contents Volume 323 Number 3 (1997)
• Springer LINK:A&A-EE: Table of Contents Volume 330 Number 3 (1998)

... By means of deep optical images obtained at the Special Astrophysical Observatory 6-m telescope it was discovered that some Seyfert galaxies that were earlier considered to be non-interacting objects displayed signatures of elongated tidal envelopes belonging to satellite debris. ... Our results suggest that statistic studies based on popular imaging surveys (for example SDSS) can lead to an underestimation of the fraction of minor mergers among galaxies with active nuclei (AGN). ...

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• A unique isolated dwarf spheroidal galaxy KKR25
• Measurement of the dark halo shape in polar ring galaxies
• topic_en

... 2008 November 4 . The Double Ring Galaxies of Arp 147 from Hubble . ... Explanation: How could a galaxy become shaped like a ring? ... This blue galaxy is part of the interacting galaxy system known as Arp 147 , and shows a ring because it has recently collided with the other galaxy in the frame, the red galaxy on the left. Unusually, even this red galaxy shows a ring like band, although it is seen nearly edge-on. ... About APOD | ...

Еще в разделе: (Показать все результаты (>3425) - www.sai.msu.su/ )

• APOD: July 28, 1995 - M82: An Irregular Galaxy
• APOD: 2005 October 22 - Ring Galaxy AM 0644-741 from Hubble
• APOD: 2015 April 19 - Ring Galaxy AM 0644 741 from Hubble