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Physical Properties and Abundances of Novae in the Nebular Phase

Published online by Cambridge University Press:  12 April 2016

M.A.J. Snijders
M.A.J. Snijders*
Affiliation:
Astronomisches Institut Tübingen

Abstract

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We discuss the derivation and behaviour of temperatures and densities of nova ejecta during the nebular stage. A systematic comparison is made between fairly complete sets of abundances for 3 C/O and 2 Neon novae. The abundances in the ejecta might influence the formation and composition of circumstellar dust in novae.

Type
1c. Nebular Ejecta
Information
International Astronomical Union Colloquium , Volume 122: Physics of Classical Novae , 1990 , pp. 188 - 194
Copyright
Copyright © Springer-Verlag 1990

References

[1] Shaia, M.M., 1989, Pub. Astr. Soc. Pacif.. 101. 5.Google Scholar
[2] Starrfield, S., and Snijders, M.A.J., 1987, in “Exploring the Universe with the IUE Satellite”, Kondo, Y. ed., D. Reidel Publishing Company, p377.CrossRefGoogle Scholar
[3] Truran, J.W. and Livio, M., 1986, Astrophys.J., 308. 721.Google Scholar
[4] Boggess, A. et al., 1978, Nature, 275, 377.Google Scholar
[5] Gallagher, J.S., Hege, E.K., Kopriva, D.A., Williams, R.E. and Butcher, H.R., 1980, Astrophys.J, 227, 55.Google Scholar
[6] Williams, R.E., Woolf, N.J., Hege, E.K., Moore, R.L. and Kopriva, D.A., 1978, Astrophys.J., 224. 171.Google Scholar
[7] Williams, R.E., 1982, Astrophys.J., 261. 170.Google Scholar
[8] Hassall, B.J.M., et al., 1989, preprint, to be submitted to Mon.Not.R. astr.Soc.Google Scholar
[9] Snijders, M.A.J., Batt, T.J., Roche, P.F., Seaton, M.J., Morton, D.C., Spoelstra, T.A.T. and Blades, J.C., 1987, Mon. Not. R. astr. Soc. 228. 329.CrossRefGoogle Scholar
[10] Stickland, D.J., Penn, C.J., Seaton, M.J., Snijders, M.A.J. and Storey, P.J., 1981, Mon. Not. R. astr. Soc. 197. 107.Google Scholar
[11] Storey, P.J., 1981, Mon.Not.R.astr.Soc. 195, 27P.Google Scholar
[12] Williams, R.E., Ney, E.P., Sparks, W.M., Starrfield, S.G., Wyckoff, S. and Truran, J.W., 1985, Mon. Not. R. astr. Soc. 212, 753.Google Scholar
[13] Snijders, M.A.J., Batt, T.J., Seaton, M.J., Blades, J.C., Morton, D.C., 1984, Mon. Not. R. astr. Soc. 211, 7P.Google Scholar
[14] Hassall, B.J.M., et al., 1989, this volume.Google Scholar
[15] Krautter, J. and Williams, R.E., 1989, Astrophys.J., 341. 968.Google Scholar
[16] Andrea, J. and Drechsel, H., 1989, this volume.Google Scholar
[17] Nussbaumer, H. and Storey, P.J., 1984, Astr. Astrophys. Suppl., 56, 293.Google Scholar
[18] Osterbrock, D.E., 1974, in “Astrophysics of Gaseous Nebulae”, W.H. Freeman and Company, San Francisco.Google Scholar
[19] Krautter, J. et al., 1984, Astr. Astrophys., 137. 307.Google Scholar
[20] Bohigas, J., Echevarria, J., Diego, F., Sarmiento, J.A., 1989, Mon.Not.R.astr.Soc. 228, 1395.Google Scholar
[21] Ferland, G.J. and Shields, G.A., 1978, >Astrophysc J., 226. 172.Astrophysc+J.,+226.+172.>Google Scholar
[22] Ferland, G.J., Lambert, D.L. and Woodman, J.A., 1986, Astrophys.J.Suppl., 60, 375.Google Scholar
[23] Joy, A.H., 1961, AstrophysJ., 133. 493.Google Scholar
[24] Mendoza, C., 1983, in “Planetary Nebulae”, Flower, D.R., Ed., IAU symposium 103, pl43.Google Scholar
[25] Wamsteker, W. et al., 1989, Astron.Astrophys. Suppl., 79, 1.Google Scholar
[26] Cameron, A.G.W., in “Essays in Nuclear Astrophysics”, eds. Barnes, C.A., Clayton, D.D. and Schramm, D.N., (Cambridge: Cambridge Univ. Press), p23.Google Scholar
[27] Lance, C.M., McCall, M.L. and Uomoto, A.K., 1988, Astrophys.J.Suppl., 66, 151.Google Scholar
[28] Penn, C.J., Snijders, M.A.J., Stickland, D.J. and Kitchin, C.R., 1989, submitted to Mon. Not. R. astr. Soc.,Google Scholar
[29] Williams, R.E., 1985, in “Production and distribution of C,N,O elements”, eds. Danziger, I.J. et al., p 225.Google Scholar
[30] Gehrz, R.D., Grasdalen, G.L. and Hackwell, J.A., 1985, Astrophys.J.Lett., 298, L47.Google Scholar
[31] Gehrz, R.D., Grasdalen, G.L., Greenhouse, M., Hackwell, J.A., Hayward, T. and Bentley, A.F., 1986, Astrophys.J.Lett., 308, L63.Google Scholar
[32] Catchpole, R.M., Glass, I.S., Roberts, G., Spencer Jones, J and Whitelock, P.A., 1985, South African Astr. Obs. Circ. 9, 1.Google Scholar
[33] Whitelock, P.A. et al., 1984, Mon. Not. R. astr. Soc. 211. 421.Google Scholar
[34] Wiescher, M., Gorres, J., Thielmann, F.-K. and Ritter, H., 1986, Astron.Astrophys., 160. 56.Google Scholar
[35] Law, W.Y. and Ritter, H., 1983, Astron.Astrophys., 123. 33.Google Scholar
[36] Starrfield, S., 1987, in “New insights in Astrophysics”, ed. Rolfe, E., ESA SP-263, p239.Google Scholar