Results 191 to 200 of about 43,402 (211)
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Dynamics of Disk Galaxies (Invited Review)
Astrophysics and Space Science, 1986In order to detect the gravitational effect of the dark corona component of disk galaxies, it is necessary to have surface photometry and rotation data that extend well beyond three disk-scale lengths. Such data exists now for several pure disk galaxies. There is very strong evidence for dark coronas in these galaxies.
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Stability of disk-like galaxies – Part II: The Kuzmin disk
Analysis, 2007SummaryWe prove the existence and nonlinear stability of the Kuzmin disk, a polytropic steady state of the Vlasov–Poisson system widely used in astrophysics, which has infinite support, but finite mass. As in Part I we use the variational approach by REIN and GUO.
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A cold, massive, rotating disk galaxy 1.5 billion years after the Big Bang
Nature, 2020Marcel Neeleman +2 more
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Mapping Metallicity Variations across Nearby Galaxy Disks
Astrophysical Journal, 2019I-Ting Ho, Brent Groves, Eva Schinnerer
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The Two Young Star Disks in the Central Parsec of the Galaxy: Properties, Dynamics, and Formation
Astrophysical Journal, 2006Reinhard Genzel, Jorge Cuadra
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Supermassive black holes do not correlate with galaxy disks or pseudobulges
Nature, 2011John Kormendy
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CLUMPY DISKS AS A TESTBED FOR FEEDBACK-REGULATED GALAXY FORMATION
Astrophysical Journal Letters, 2016Lucio Mayer +2 more
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