... Дни открытых дверей к юбилею САО РАН (12-14 апреля 2016 г.) . Международная конференция "Dark Ages and White Nights (Spectroscopy of the CMB)" (20-24 июня 2016 г.) . ... Международная конференция MULTI-SPIN GALAXIES - 2016 (26-30 сентября 2016 г.) . Международная астрономическая конференция "Физика звезд: от коллапса до коллапса" (3-7 октября 2016 г.) Архив . ... Подробнее.. ... 10.02.16 . ... БТА в реальном времени . ... Цейсс-1000 в реальном времени . ... Последнее обновление: 22/03/2016 ...

. Back to A.Zasov's homepage.

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. ...

... 145Slee,Roy Savage We present detailed radio and optical parameters for the stronger radio sources in 58 Abell cluster fields observed with the Very Large Array (VLA) using scaled arrays at 1.5 and 4.9 GHz. ... The cluster fields were distributed over 24 h of RA and between declinations +35 deg and -30 deg. ... Optical identifications Cluster Source Radio Centroid Optical Position EF Ang. ...

... 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 . ...

... 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. ...

Next: Other Galaxies with HI Up: Galaxies with Broad HI Previous: NGC 7582 . Table 4 lists a few strongly interacting or merging galaxies which also show broad H I absorption lines. ... Table: Strongly interacting pairs of spirals . ... But in these galaxies the cold gas which feeds the starburst is driven inwards by strong tidal interaction or merging between galaxies (see e.g., Rieke et al. 1985), whereas in the nearby galaxies, bars and/or weak galaxy interactions may be responsible. ...

Astronomy Discussion Forums . Forums: . Atm ћ Astrophotography ћ Blackholes ћ Blackholes2 ћ CCD ћ Celestron ћ Domes ћ Education . ... Discussion Forums . ... Brightest Northern Hemisphere Galaxy . Forum List | ... Post Message | ... In which constellation would I find the brightest galaxy in the northern hemisphere? ... www.astronomy.net . ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

This is an image of the Galaxy NGC3877 and the supernova 1998S in the constellation Ursa Major. ... As others have posted, the supernova is actually easier to see than the parent galaxy. I was able to see it when I was done imaging last night (3/28/98) with the Fastar 8 SCT at 221X . ... Back to Supernovae in NGC and IC galaxies . Back to Supernova 1998S images . David Bishop Last modified: Tue Oct 6 15:40:58 EDT 1998 ...

... Some 60 million light-years away in the southerly constellation Corvus, two large galaxies collided. But the stars in the two galaxies cataloged as NGC 4038 and NGC 4039 don't collide in the course of the ponderous, billion year or so long event. ... Spiral Galaxy NGC 3190 Almost Sideways . ... Some spiral galaxies are seen almost sideways. ... The Coma Cluster of Galaxies . ... Virgo Cluster Galaxy NGC 4731 . ... Barred spiral galaxy NGC 4731 lies some 65 million light-years away. ...

. Back to Home . radiative transfer studies in the dawn . of a new generation of observing facilities . May 14-16, 2007 . Het Pand - Ghent - Belgium . Pictures of the workshop . Pictures from Andreas Lundgren . Pictures from Karl Gordon . Pictures from Simone Bianchi . Pictures from Maarten Baes . Back to Home .

... Black holes are found at the centres of galaxies which are similar in size to our own Milky Way Galaxy or larger. When black holes collide and merge they form supermassive black holes which are events among the most powerful in the universe. ... 55, No. 1, pages 1-5, 'Observational Effects of Strong Gravity in Vicinity of Supermassive Black Holes' . ... International Year of Astronomy, Ireland National Node . ...

... The color composite image of Centaurus A reveals the lobes and jets emanating from the active galaxy?s central black hole. ... Astronomers have a new insight into the active galaxy Centaurus A (NGC 5128), as the jets and lobes emanating from the central black hole have been imaged at submillimetre wavelengths for the first time. ... Centaurus A hosts a very active and highly luminous central region, caused by the presence of a supermassive black hole is the source of strong radio and X-ray emission....

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 . ...

... fran?ais . ... Back when the first stars and galaxies formed, the Universe was filled with a thick fog of hydrogen gas. However, the Universe?s first galaxies were full of huge stars that gave off very strong Ultra Violet or UV light. ... What we know little about, are the first galaxies. Up to now our telescopes have only been able to see them as very faint blobs, as shown in the picture above. ... Observations like this will help astronomers to investigate how the first galaxies were formed. ...

. 30 Nov. - 5 Dec. 1998 . Organized by Instituto de Astrofisica de Canarias , Tenerife, Spain. 1. 2. 3. 4. 5. 6. 7. 8. 9. 10. 11. 12. 13. 14. 15. 16. 17. 18. 19. 20. 21. 22. 23. 24. 25. 26. 27. 28. This homepage is a part of Sternberg Astronomical Institute WWW-area.

... 2005 March 4 . NGC 1427A: Galaxy in Motion . Credit: Hubble Heritage Team ( AURA / STScI ), ESA , NASA . Explanation: In this tantalizing image , young blue star clusters and pink star-forming regions abound in NGC 1427A, a galaxy in motion. ... Still, it is understood that interactions with cluster gas and the other cluster galaxies during its headlong flight will ultimately disrupt galaxy NGC 1427A . ... About APOD | ... NASA Web Site Statements, Warnings, and Disclaimers . ...

HST optical image 0.8 microns . The Experiment: AGN and galaxy evolution . A small fraction of galaxies contain an “Active Nucleus” (AGN) ? probably a supermassive black hole ? gas falls towards BH (accretion) ? ... AGN in some emits two jets of plasma ? ... Immense power of AGN ? do the modify evolution of galaxy . ... High resolution telescopes to probe the working of the AGN . Previous slide . Next slide . Back to first slide . ...

... RC0907+0436 , RC0908+0451 , RC0934+0505 , RC0942+0447 , RC0945+0454 . ... RC1011+0502 , RC1031+0443 , RC1043+0440 , RC1051+0449 . ... RC1113+0436 , RC1142+0455 , RC1148+0456 , RC1152+0449 , RC1154+0431 , . ... RC1429+0501 , RC1436+0501 , RC1439+0455 , RC1446+0508 . ... RC1503+0456 , RC1510+0438 , RC1551+0458 . ... RC1609+0456 , RC1626+0448 , RC1638+0450 , RC1646+0501 . ... RC1703+0502 , RC1706+0502 , RC1720+0455 , RC1722+0442 , RC1725+0457 , RC1735+0454 , RC1740+0502 . ...

. First page Back Continue Last page Overview Graphics .