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http://www.atnf.csiro.au/research/conferences/2012/boltonsymp/programme_v5.pdf.

1. The Galaxy Gallery: Messier Objects
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 . ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/messier.html -- 7.0 Кб -- 23.07.2004
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2. Research
... Structure and evolution of galaxies . The Magellanic Stream and high-velocity clouds . ... DINGO the ASKAP deep H i survey . ... In this scenario, small dark-matter haloes are expected to form first and later merge and accrete onto larger haloes to form more massive galaxies like the Milky Way. ... Our Milky Way is surrounded by a vast population of gas clouds, called high-velocity clouds (HVCs), that are mainly detectable in H i emission. ... Compact high-velocity clouds around the Milky Way . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Tobias.Westmeier/research.php -- 9.0 Кб -- 09.04.2016
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3. Finding Your Way in the Milky Way | Astronotes
... Milky Way . ... Map of the Milky Way (based on data from NASA's Spitzer Space Telescope) showing its two major stellar arms and central bar. ... ТљIn written science fiction, one often encounters another navigational convention, where towards the Galactic Centre is described as т??Corewardт??, away from the Centre towards the rim of the Milky Way is т??Rimwardт??, objects in the direction of the Galaxyт??s rotation are т??Spinwardт??, while objects in the opposite direction are т??antispinwardт?? ...
[ Сохраненная копия ]  Ссылки http://www.armaghplanet.com/blog/finding-your-way-in-the-milky-way.html -- 47.4 Кб -- 09.04.2016
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5. APOD: 2001 December 19 - Finding Dark Matter
... 2001 December 19 . Finding Dark Matter . ... Explanation: Where is dark matter ? Galaxies rotate and move in clusters as if a tremendous amount of unseen matter is present. ... In the above frame from a computer simulation of our universe , a 300 million light-year slice shows dark matter in gray and galaxies as colored circles. The red box indicates the location of a rich cluster of galaxies , while the green box shows a more typical cross-section of our universe . ... About APOD | ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap011219.html -- 5.1 Кб -- 01.10.2012
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6. ADS Abstract Service Results
Find Similar Abstracts . ... The origin and evolution of galaxies and stars . ... GALACTIC EVOLUTION, STELLAR EVOLUTION, BLACK HOLES (ASTRONOMY), GALACTIC NUCLEI, NEUTRON STARS, PULSARS, QUASARS, STAR CLUSTERS, STELLAR SYSTEMS, WHITE DWARF STARS . ... Current views on the formation and evolution of galaxies, stars, and various types of stellar systems are surveyed, with evolution traced from the superdense primordial fireball through to white dwarfs, neutron stars, and black holes. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~mystery/html/Z/biblio/76.5.html -- 6.7 Кб -- 29.05.1996
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7. Finding Dark Matter
... Galaxies rotate and move in clusters as if a tremendous amount of unseen matter is present. But does dark matter exist in the greater universe too -- and if so, where? ... In the above frame from a computer simulation of our universe , a 300 million light-year slice shows dark matter in gray and galaxies as colored circles. ... Publications with keywords: universe - dark matter - 2dF survey - simulation . Publications with words: universe - dark matter - 2dF survey - simulation . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/1173934 -- 16.3 Кб -- 02.01.2002
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8. http://www.mso.anu.edu.au/seminars/abstracts/20141127-1100.html
. 6). From their rest-frame UV emission we can estimate individual star formation rates, and study evolution of the star formation rate density with cosmic time. At lower redshifts, near-infrared spectroscopy (including slitless spectroscopy with WFC3 on HST) has enabled us to measure star formation rates at redshifts beyond one through the redshifted rest-frame optical lines. I will review current work on this, and look to future developments (in particular JWST).
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20141127-1100.html -- 4.4 Кб -- 10.04.2016
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9. The history of star formation and mass assembly in early-type galaxies Bojan
... Bojan Nikolic web pages (r. 329) . Galaxy Evolution . ... By comparing narrow band spectral line indices with recent models of simple stellar populations (SSPs) we investigate trends in the star formation history as a function of galaxy mass (velocity dispersion), density of environment and galactic radius. ... MJD of the SDSS observation of the galaxy . ... The history of star formation and mass assembly in early-type galaxies . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/galevol/clemensetal08.html -- 11.5 Кб -- 04.04.2016