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The epochs of bulge and disk formation
1994
Open Astronomy
To understand the evolution of galaxies, particularly in the early stages, it is fundamental to investigate the different components of a galaxy and the interactions between them. The number of components and, even more important, the number of processes that account for mass, momentum and energy transfer between the components make it impossible to describe galactic evolution with simple analytical models. Especially in the case of rotating galaxies, a twodimensional hydrodynamical treatment
doi:10.1515/astro-1994-1-218
fatcat:zry246jdpnczfonkz5gxuicggi