Abstract
A kinetic description of the equilibrium structure of accretion disc plasma is presented. It is possible to have an equilibrium configuration for a stationary axisymmetric gravitating plasma disc with spatial gradients in density, temperature and drift speed of plasma particles.
Similar content being viewed by others
References
Bhaskaran, P. and Prasanna, A.R.: 1989,Astrophys. Space Sci. 159, 109.
Bhaskaran, P. and Prasanna, A.R.: 1990a,Astrophys. Astro. 11, 49.
Bhaskaran, P., Thripathy, S.C., and Prasanna, A.R.: 1990b,J. Astrophys. Astron. 11, 461.
Bisnovathy Kogan, G.S. and Binnikov, S.I.: 1972,Astrophys. Space Sci. 19, 119.
Ichimaru, S.: 1977,Astrophys. J. 214, 840.
Krishan, V., Sreedharan, T.D., and Mahajan, S.M.: 1991,Monthly Notices Roy. Astron. Soc. 249, 596.
Mahajan, S.M.: 1989,Phys. Fluids, Bl 1, 43.
Prasanna, A.R. and Bhaskaran, P.: 1989,Astrophys. Space Sci. 153, 201.
Pringle, J.E. and Rees, M.J.: 1972,Astron. Astrophys. 21, 1.
Shapiro, S.L. and Lightman, A.P.: 1976,Ap. J. 204, 187.
Thorne, K.S. and Price, R.H.: 1975,Ap. J. (Letters) 195, L101.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Bhaskaran, P., Krishan, V. Kinetic equilibria of accretion discs. Astrophys Space Sci 232, 65–78 (1995). https://doi.org/10.1007/BF00627544
Received:
Accepted:
Issue Date:
DOI: https://doi.org/10.1007/BF00627544