Flat rotation curves according to the fragmentation/shear flow model of galaxy formation
- 1 January 1984
- journal article
- Published by Springer Nature in Astrophysics and Space Science
- Vol. 105 (1) , 109-130
- https://doi.org/10.1007/bf00651212
Abstract
No abstract availableKeywords
This publication has 25 references indexed in Scilit:
- Fragmentation of the universeAstrophysics and Space Science, 1983
- 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
- The distribution of luminosity in spiral galaxiesThe Astrophysical Journal Supplement Series, 1981
- A model of the formation of spherical galaxiesAstrophysics and Space Science, 1980
- A model of the formation of spiral galaxiesAstrophysics and Space Science, 1980
- A model of the formation of elliptical galaxiesAstrophysics and Space Science, 1978
- A simple model of convection in the Jovian atmosphereIcarus, 1976
- Dynamics of early type galaxies. I - The rotation curve of the elliptical galaxy NGC 4697The Astrophysical Journal, 1975
- A galactic formation model based on post-big bang fragmentationAstrophysics and Space Science, 1972
- On the Distribution Ofmass in Galaxies. I. The Large-Scale Structure of Ordinary Spirals with Applications to M 31.The Astrophysical Journal, 1960