A possible scenario for the morphological differentiation of galaxies

Details A possible scenario for the morphological differentiation of galaxies A possible scenario for the morphological differentiation of galaxies

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mmsai..50..165d&link_type=abstract

(Workshop on Chemical Inhomogeneities in the Galaxy, Frascati, Italy, May 29-June 2, 1978.) Società Astronomica Italiana, Memori

Astronomy and Astrophysics

Astronomy

Astronomical Models, Cosmology, Galactic Evolution, Chemical Evolution, Disk Galaxies, Elliptical Galaxies, Galactic Structure, Gravitational Collapse, Spiral Galaxies, Time Response

Scientific paper

Developing an idea by Di Fazio and Occhionero (1978), it is shown that the initial conditions (repartition of energy between rotation and thermal content) determine whether the following evolution of a protogalaxy will be dissipative or not. In the latter limiting case, the system will only have a spheroidal component, thus forming an elliptical, while in the first case the system will develop a disk (thus forming a spiral or an SO galaxy).

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