Hostname: page-component-76fb5796d-x4r87 Total loading time: 0 Render date: 2024-04-26T09:03:53.815Z Has data issue: false hasContentIssue false
  • English
  • Français

Advances in Numerical Simulations of Gaseous Nebulae

Published online by Cambridge University Press:  07 August 2017

Gary J. Ferland
Gary J. Ferland*
Affiliation:
Department of Physics & Astronomy, University of Kentucky, Lexington, KY 40506, USA Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatories, Casilla 603, La Serena, Chile

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

I outline recent advances in numerical simulations of gaseous nebulae. These fall into three major areas; the Opacity Project and its extensions, the role of grains within the ionized gas, and the effects of mechanical heat on the nebula. These advances, together with improvements in stellar atmosphere calculations, should lead to a new generation of more realistic simulations of conditions in planetary nebulae and predictions of their emitted spectra.

Type
III. Highlights on the Nebulae
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 123 - 130
Copyright
Copyright © Kluwer 1993 

References

Ashley, M., and Hyland, A.R., 1988, Ap. J. 331, 532.CrossRefGoogle Scholar
Baldwin, J., Ferland, G.J., Martin, P.G., Corbin, M., Cota, S., Peterson, B.M., and Slettebak, A., 1991, Ap. J. 374, 580.CrossRefGoogle Scholar
Borkowski, K.J., and Harrington, J.P., 1991, Ap. J. 379, 168.CrossRefGoogle Scholar
Cowie, L.L., and Sangila, A., 1986, Ann Rev Ast Ap 24, 499.CrossRefGoogle Scholar
Draine, B.T., 1978, Ap. J. (Sup) 36, 595.CrossRefGoogle Scholar
Draine, B.T., and Salpeter, E.E., 1979, Ap. J. 231, 77.CrossRefGoogle Scholar
Field, G. B., 1974, Ap. J. 187, 453.CrossRefGoogle Scholar
Grevesse, N., and Anders, E., 1989, Cosmic Abundances of Matter , AIP Conference Proceedings 183, Ed. Waddington, C. J., (New York: AIP).Google Scholar
Ferland, G.J. and Persson, S.E., 1989, Ap. J. 347, 656.CrossRefGoogle Scholar
Harrington, J.P., 1990, Planetary and Proto-Planetary Nebulae, from IRAS to ISO , ed. Martinez, P, p 277.Google Scholar
Harrington, J.P., 1989, Planetary Nebulae , IAU 131, ed. Torres-Peimbert, S., p 157.CrossRefGoogle Scholar
Harrington, J.P., and Feibelman, W.P., 1984, Ap. J. 277, 716.CrossRefGoogle Scholar
Kingdon, J., and Ferland, G.J., 1993, Ap. J. submitted.Google Scholar
Lame, N.J., and Ferland, G.J., 1991, Ap. J. 367, 208.CrossRefGoogle Scholar
Middlemass, D., Clegg, R.E.S., Walsh, J.R., and Harrington, J.P., 1991, MNRAS 251, 284.CrossRefGoogle Scholar
Nahar, S.N., and Pradhan, A.K., 1992a, Phys Rev in press.Google Scholar
Nahar, S.N., and Pradhan, A.K., 1992b, Ap. J. 397, 729.CrossRefGoogle Scholar
Oliveira, S., and Maciel, W.J., 1986, Astro Space Sci 126, 211.CrossRefGoogle Scholar
Osterbrock, D.E., 1989, Astrophysics of Gaseous Nebulae and Active Galactic Nuclei , University Science Press.CrossRefGoogle Scholar
Pequignot, D., 1983, in Planetary Nebulae , IAU 103, Flower, D., ed., p 173.CrossRefGoogle Scholar
Pequignot, D., 1986, Workshop on Model Nebulae , p 363, Pub. de l'Observatoire de Paris.Google Scholar
Reilman, R.F., and Manson, S.T., 1979, Ap. J. Sup. 40, 815.CrossRefGoogle Scholar
Seaton, M.J., 1987, J. Phys. B 20, 6363.CrossRefGoogle Scholar
Shields, G.A., 1975, Ap. J. 195, 475.CrossRefGoogle Scholar
Spitzer, L., 1948, Ap. J. 107, 6.CrossRefGoogle Scholar
Stoy, R.H., 1933, MNRAS 93, 588.CrossRefGoogle Scholar