Dissipative processes, galaxy formation and 'early' star formation

Details Dissipative processes, galaxy formation and 'early' star formation Dissipative processes, galaxy formation and 'early' star formation

Mar 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978phys...17..371r&link_type=abstract

(Niels Bohr Institut, Teknisk Videnskabelige Forskningsrad, and Nordisk Institut for Teoretisk Atomfysik, Symposium on Quasars a

Astronomy and Astrophysics

Astrophysics

13

Astronomical Models, Cosmic Rays, Cosmology, Galactic Clusters, Galactic Evolution, Halos, Missing Mass (Astrophysics), Optical Thickness, Quasars, Stars

Scientific paper

Scenarios are described for the process whereby the primordial material
is transformed from gas at z approximately equal to 1000 into bound
systems and stars at the present epoch. The alleged 'missing mass' could
consist of stars which condensed at z approximately greater than 100
before galaxies had formed as gravitationally bound units

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