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Amaro-Seoane, P. and Spurzem, R. (2001).
Gas in the Central Regions of AGN: The Interstellar Medium and
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In ASP Conf. Ser. 249: The Central Kiloparsec of Starbursts and
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Amaro-Seoane, P. and Spurzem, R. (2004).
Dense Gas-Star Systems: Evolution of Supermassive Stars.
In In "Carnegie Observatories Astrophysics Series, Vol. 1:
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Bettwieser, E. and Spurzem, R. (1986).
Anisotropy in stellar dynamics.
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Binney, J. and Tremaine, S. (1987).
Galactic Dynamics.
Princeton University Press.
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Castor, J. I. (1972).
Radiative Transfer in Spherically Symmetric Flows.
apj, 178:779-792.
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Giersz, M. and Spurzem, R. (1994).
Comparing direct -body integration with anisotropic gaseous models
of star clusters.
MNRAS, 269:241.
- Henyey et al., 1959
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Henyey, L. G., Wilets, L., Böhm, K. H., Lelevier, R., and Levee,
R. D. (1959).
A Method for Atomic Computation of Stellar Evolution.
ApJ, 129:628.
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Kippenhahn, R. and Weigert, A. (1994).
Stellar Structure and Evolution.
Springer-Verlag Berlin Heidelberg.
- Langbein et al., 1990
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Langbein, T., Fricke, K. J., Spurzem, R., and Yorke, H. W. (1990).
Interactions between stars and gas in galactic nuclei.
aa, 227:333-341.
- Lin and Tremaine, 1980
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Lin, D. N. C. and Tremaine, S. (1980).
A reinvestigation of the standard model for the dynamics of a massive
black hole in a globular cluster.
ApJ, 242:789-798.
- Louis and Spurzem, 1991
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Louis, P. D. and Spurzem, R. (1991).
Anisotropic gaseous models for the evolution of star clusters.
MNRAS, 251:408-426.
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Lynden-Bell, D. and Eggleton, P. P. (1980).
On the consequences of the gravothermal catastrophe.
MNRAS, 191:483-498.
- Rosenbluth et al., 1957
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Rosenbluth, M. N., MacDonald, W. M., and Judd, D. L. (1957).
Phys. Rev. 2nd Ser., 107:1.
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Spitzer, L., J. and Saslaw, W. C. (1966).
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ApJ, 143:400.
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Spitzer, L. (1987).
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Princeton University Press.
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Spurzem, R., Berczik, P., Hensler, G., Theis, C., Amaro-Seoane, P.,
Freitag, M., and Just, A. (2003).
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ArXiv Astrophysics e-prints.
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Yorke, H. W. (1980).
Numerical solution of the equation of radiation transfer in
spherical geometry.
aa, 86:286-294.
Pau Amaro-Seoane
2005-02-25