... of clumps in the ring position at tenuates a lot of the radiation coming from the half of the galaxy below the plane, acting ... Clumps have been randomly distributed according to the ringlike distribution of molecular gas observed in our Galaxy. ...
... galaxy formation and evolution within the Ю?-CDM paradigm can be tested against ... SECCO1 would be a new faint dwarf galaxy residing in the Virgo cluster of galaxies ... galaxy, it would be an extremely gas-dominated and star-poor one, akin to the ...
... Dramatic evidence of this is illustrated in our neighboring galaxy, the Large Magellanic Cloud (LMC), by the above ring shaped nebula , Henize 70 (also known as N70 and DEM301 ). ...
... Effects of Clumping on the Observed Properties of Dusty Galaxies . ... Carlo radiative transfer simulations for spiral galaxies modelled as a stellar disk ... the observed properties of Giant Molecular Clouds and molecular gas in the Galaxy ...
... SN1987A occurred in the Large Magellanic Cloud (LMC), a satellite galaxy only 150,000 light years from our Milky Way Galaxy . ... The rings of SN1987A are currently excited by light from the initial explosion. ...
... galaxies host a supermassive black hole (BH) in their centre with a mass between 10 ... galaxy is suggested by the observed correlation between the BH mass and the stellar ...
... Rest-frame ultraviolet (UV) and optical Hubble Space Telescope images obtained by Pentericci et al. (1999, 2001) show a bright ... a study of the absorption lines in the rest-frame UV spectrum of one such galaxy: the z = 2.63 radio galaxy MRC 2025-218 ...
... Lyman Break Galaxies are objects selected based on the Ly-break technique and based on their UV rest-frame blue color. ... given that the latter sample includes not only rest-frame UV selected galaxies, but also near- and mid-IR selected, and that ...
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Ссылки http://www.arcetri.astro.it/~marconi/TESI/AlessioGnerucci_PhD.pdf -- 2597.9 Кб -- 02.02.2012 Похожие документы