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Lecture 3 - Formation of Galaxies What processes lead from the tiny fluctuations which we see on the surface of last scattering, to the diverse galaxies.
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Galaxies, Cosmology and the SKA Catherine Cress (UWC)
Cosmology beyond the standard model Multi component dark matter model A. Doroshkevich, Astro-Space Center, FIAN, Moscow, Russia M. Demianski, University.
Physics 133: Extragalactic Astronomy and Cosmology Lecture 15; March 5 2014.
Cosmology beyond the standard model Multi component dark matter model
Physics 133: Extragalactic Astronomy and Cosmology
Eloisa Menegoni ICRA and INFN, University of Rome “La Sapienza”
m Thesis
