Abstract
The present analytical model describes the collapse of a protogalactic cloud under the influence of gravitational and viscous forces. The model provides a discriminating mechanism that dictates what type of galaxy will eventually form.
Similar content being viewed by others
References
Brown, W. K.: 1972,Astrophys. Space Sci. 15, 293.
Brown, W. K.: 1978,Astrophys. Space Sci. 54, 365.
Brown, W. K.: 1980,Astrophys. Space Sci. 72, 15.
Brown, W. K.: 1981,Spec. Sci. Tech. 4, 415.
Brown, W. K.: 1984,Astrophys. Space Sci. 105, 109.
Brown, W. K.: 1985,Astrophys. Space Sci. 111, 139.
Brown, W. K. and Gritzo, L. A.: 1980,Astrophys. Space Sci. 70, 493.
Brown, W. K., Karp, R. R., and Grady, D. E.: 1983,Astrophys. Space Sci. 94, 401.
Fillmore, J. A. and Goldreich, P.: 1984,Astrophys. J. 281, 1.
Freeman, K. C.: 1970,Astrophys. J. 160, 811.
Grady, E. E. and Kipp, M. E.: 1985,J. Appl. Phys. (in press).
Hogan, C. J.: 1982,Astrophys. J. 252, 418.
Marion, J. B.: 1970, inClassical Dynamics of Particles and Systems, 2nd ed., Acadmic Press,New York.
Ozernoy, L. M.: 1974, in M. S. Longair (ed.), ‘Confrontations of Cosmological Theories with Observational Data’,IAU Symp. 79, 227.
Seiden, P. E.: 1983,Astrophys. J. 266, 555.
Seiden, P. E., Schulman, L. S., and Elmegreen, B. G.: 1984,Astrophys. J. 282, 95.
Shaya, E. J. and Tully, R. B.: 1984,Astrophys. J. 281, 56.
Takase, B. and Kinoshita, H.: 1967,Publ. Astron. Soc. Japan 19, 409.
Vettolani, G., Marano, B., Zamorani, G., and Bergamini, R.: 1980,Monthly Notices Roy. Astron. Soc. 193, 269.
Author information
Authors and Affiliations
Additional information
Los Alamos National Laboratory is operated by the University of California for the United States Department of Energy under Contract W-7405-ENG-36.
Rights and permissions
About this article
Cite this article
Brown, W.K. A model of protogalactic cloud collapse. Astrophys Space Sci 113, 143–153 (1985). https://doi.org/10.1007/BF00650277
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00650277