Approximate rotation curve solutions for the evolution of a viscous protogalactic disk
- 1 January 1985
- journal article
- Published by Springer Nature in Astrophysics and Space Science
- Vol. 111 (1) , 139-155
- https://doi.org/10.1007/bf00651524
Abstract
No abstract availableKeywords
This publication has 16 references indexed in Scilit:
- A galactic disk is not a true exponentialThe Astrophysical Journal, 1984
- The angular momentum content of galaxiesThe Astrophysical Journal, 1984
- The role of the gas in propagating star formationThe Astrophysical Journal, 1983
- Rotational properties of 23 SB galaxiesThe 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
- A model of the formation of spherical galaxiesAstrophysics and Space Science, 1980
- Rotational properties of 21 SC galaxies with a large range of luminosities and radii, from NGC 4605 /R = 4kpc/ to UGC 2885 /R = 122 kpc/The Astrophysical Journal, 1980
- A model of the formation of elliptical galaxiesAstrophysics and Space Science, 1978
- A galactic formation model based on post-big bang fragmentationAstrophysics and Space Science, 1972
- On the Disks of Spiral and so GalaxiesThe Astrophysical Journal, 1970