... The Sombrero Galaxy in Infrared . ... 11.03.2012 . ... SSC , JPL , Caltech , NASA Explanation: This floating ring is the size of a galaxy. ... The dark band of dust that obscures the mid-section of the Sombrero Galaxy in optical light actually glows brightly in infrared light. ... The Sombrero Galaxy, also known as M104 , spans about 50,000 light years across and lies 28 million light years away. ... Publications with keywords: Sombrero galaxy - M 104 . ... Sombrero Galaxy Across the Spectrum . ...

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• Астронет > The Sombrero Galaxy in Infrared

... 2006 May 24 . A Five Quasar Gravitational Lens . ... Explanation: What's happening near the center of this cluster of galaxies? ... In reality, an entire cluster of galaxies is acting as a gigantic gravitational lens that distorts and multiply-images bright objects that occur far in the distance. ... Close inspection of the above image will reveal that the arced galaxies at 2 and 4 o'clock are actually gravitationally lensed images of the same galaxy. ... About APOD | ...

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• APOD: 2005 May 11 - The Sombrero Galaxy in Infrared
• APOD: 2015 October 4 - The Sombrero Galaxy in Infrared
• APOD: 2012 March 11 - The Sombrero Galaxy in Infrared

... May 25, 1998 . M83: A Barred Spiral Galaxy . ... Explanation: M83 is a bright spiral galaxy that can be found with a small telescope in the constellation of Hydra . M83 is a member of the Centaurus group of galaxies, a nearby group dominated by the massive galaxy Centaurus A . ... The spiral arms are given a blue color by the many bright young stars that have recently formed there. Dark dust lanes are also visible. ... About APOD > . ...

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• APOD: December 6, 1999 - M83: The Southern Pinwheel Galaxy from VLT
• APOD: October 16, 1995 - Starburst Galaxy M94
• APOD: August 7, 1998 - M65 Without Moth

Supernova 2005ew in anonymous galaxy . This page is devoted to information on Supernova 2005ew in an anonymous galaxy. Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . Information on the original web pages for many of these images can be found on the updates and links web pages. ... Most of the supernovae found by the Nearby Supernova Factory are faint and almost impossible to find. ... JM Llapasset image . ... mirror . ...

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• Supernova 1999ab in anonymous galaxy
• Supernova 1999X in CGCG 180-22
• Supernova 1998S in NGC 3877

D.Moss, R.Stepanov, T.G.Arshakian, R. Beck, M.Krause, D.Sokoloff, Multiscale magnetic fields in spiral galaxies: evolution and reversals, Astron. Astrophys., 537, A68, 13 pages (2012) . ... The effects of star-forming regions in galaxies need to be included when modelling the evolution of their magnetic fields, which can then be compared to future radio polarization observations. ... The injection of turbulent fields generates small-scale field structures. ...

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• Arshakian T. G., Stepanov R., Beck R., Krause M., Sokoloff D. Simulations of
• D.Moss, D.Sokoloff, R.Beck, Ram pressure effects in the galactic plane and

Lab . Main page News People . ASA . Master . Master net Homepage . ... Lomonosov Moscow State University Sternberg Astronomical Institute . ... MASTER . ... Lomonosov (ShOK) . ... About Space Monitoring Laboratory, scientific directions, instruments, contacts . People, who work in lab . Latest news and news archive . ... Bright MASTER PSN discovery in UGC06716 galaxy ATel 3767 . ... All news ...

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... I. Mean Surface Brightnesses and Integral Color Indices for Bars Gusev A.S. ================================================================================ Abstract: UBVRIJHK surface brightnesses and color indices of bars of galaxies are determined using surface photometry data for 100 barred galaxies (table1.dat). ... J0 Mean surface J0 brightness 46 A1 --- CI- CI sign 47 -50 F1.2 magn/sq.arcsec. U-B)0 (U-B)0 color index 52 -55 F1.2 magn/sq.arcsec. ...

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• Division of the Galaxy and Variable Stars
• Anna Mel'nik - My Home Page
• Trudy GAISH, vol. LXV, 1996, Abstracts in English

Next: Gravitational Wave Background from Previous: Galactic Gravitational Wave Background . ... It is intuitively clear that at frequencies above the critical ones for our Galaxy, one will detect rare bright jerks produced by coalescing white dwarfs   (at a rate of 1 per 100 year) and NS (at a rate of 1 per - year) in our Galaxy, against a background of the extragalactic stochastic GW. ... Firstly we consider GWB from close individual galaxies, and then will discuss overall extragalactic GWB. ...

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• Gravitational wave background from nearby galaxies
• Gravitational Wave Background from Individual Galaxies
• Structure of the Galaxy

... Sternberg Astronomical Institute , Moscow University . ... Present edition unites two parts of Catalogue of interacting galaxies by B.A.Vorontsov-Velyaminov: the first part (Part 1) containing 355 systems was published in 1959 [1] and the second one (Part 2) with 497 objects - in 1976 [2].Thus two published parts of Catalogue include 852 interacting systems. ... All new of them (1162 by number) were taken from the comments to the galaxies in Morphological catalogue by Vorontsov-Velyaminov et al.[ ...

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• Отдел внегалактической астрономии: ГАИШ Extra-galactic astronomy Group

New GCVS Version (GCVS5) FileName Explanations ----------------------------------------------------------------- ReadMe This file GCVS5 The ... ------------------------------------------------------ 1- 2 I2 --- Constell [1/88]Constellation numeric code 3- 6 I4 --- Number Star number within the constellation 7 A1 --- Component *Component identification 9- 18 A10 --- GCVS * Variable ... Field is non-blank if magMin is a magnitude or amplitude given in a system other than that indicated by magCode. ...

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• http://www.sai.msu.ru/groups/cluster/gcvs/gcvs/v/sn.txt
• http://www.sai.msu.ru/gcvs/gcvs/v/readme
• General Catalogue of Variable Stars: Vols I-III (the new electronic version).

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