The possible protogalactic role of eddies in a turbulent early universe
- 1 January 1985
- journal article
- Published by Springer Nature in Astrophysics and Space Science
- Vol. 115 (2) , 257-265
- https://doi.org/10.1007/bf00653804
Abstract
No abstract availableKeywords
This publication has 13 references indexed in Scilit:
- Approximate rotation curve solutions for the evolution of a viscous protogalactic diskAstrophysics and Space Science, 1985
- Flat rotation curves according to the fragmentation/shear flow model of galaxy formationAstrophysics and Space Science, 1984
- Dark Matter, Galaxies and Globular ClustersPublished by Springer Nature ,1984
- What is the Dark Matter? Implications for Galaxy Formation and Particle PhysicsPublished by Springer Nature ,1984
- Are Massive Halos Baryonic?Published by Springer Nature ,1984
- Fragmentation of the universeAstrophysics and Space Science, 1983
- Cosmological structure produced by a phase transition near nuclear densityThe Astrophysical Journal, 1982
- 21-cm line studies of spiral galaxies. II. The distribution and kinematics of neutral hydrogen in spiral galaxies of various morphological types.The Astronomical Journal, 1981
- Extended rotation curves of high-luminosity spiral galaxies. IV - Systematic dynamical properties, SA through SCThe Astrophysical Journal, 1978
- Models for the Formation of Disc GalaxiesMonthly Notices of the Royal Astronomical Society, 1976