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Final Review

Published online by Cambridge University Press:  18 September 2017

Yervant Terzian
Yervant Terzian*
Affiliation:
Cornell University, NAIC, Ithaca, N.Y.

Extract

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What splendid laboratories have planetary nebulae been! We have heard of important observations in the ultraviolet, optical, infrared, and radio spectral ranges, all rich in astrophysical information. We are now certain that planetary nebulae represent a crucial phase of stellar evolution. We have also begun to study the fine details of the evolution of planetary nebulae and our endless aim is to understand these objects completely.

Type
Section VI: Planetary Nebulae in a Galactic and Extragalactic Context
Information
Symposium - International Astronomical Union , Volume 103: Planetary Nebulae , 1983 , pp. 487 - 499
Copyright
Copyright © Reidel 1983 

References

Aller, L.H., and Czyzak, S.J., 1982, Preprint.Google Scholar
Boggess, A., Feibelman, W.A., and McCracken, C.W., 1981, The Universe at Ultraviolet Wavelengths, NASA-CP2171, ed. Chapman, R. Google Scholar
Feibelman, W.A., Boggess, A., Hobbs, R.W., and McCracken, C.W., 1980, Ap. J. 241, 725.CrossRefGoogle Scholar
Feibelman, W.A., 1981, PASP, 93, 719.CrossRefGoogle Scholar
Feibelman, W.A., Boggess, A., McCracken, C.W., and Hobbs, R.W., 1981, Ap. J. 246, 807.CrossRefGoogle Scholar
Harrington, J.P., Seaton, M.J., Adams, S., and Lutz, J.H., 1982, MNRAS, 199, 517.CrossRefGoogle Scholar
Hazard, C., Terlevich, R., Morton, D.C., Sargent, W.L.W., and Ferland, G., 1980, Nature, 463.CrossRefGoogle Scholar
Heap, S.R., 1980, Bull. Am. Astr. Soc., 12, 540.Google Scholar
Jacoby, G.H., 1979, PASP, 91, 754.CrossRefGoogle Scholar
Jacoby, G.H., 1982, private communication.CrossRefGoogle Scholar
Knapp, G.R., Phillips, T.G., Leighton, R.B., Lo, K.Y., Wannier, P.G., and Wootten, H.A., 1982, Ap. J., 252, 616.CrossRefGoogle Scholar
Kwok, S., Purton, C.R., and FitzGerald, P.M., 1978, Ap. J., 219, L125.CrossRefGoogle Scholar
Longmore, A.J., 1977, private communication.Google Scholar
Louise, R., 1981, Astron. Astroph., 102, 303.Google Scholar
Loulergue, M., and Nussbaumer, H., 1976, Astron. Astroph., 51, 163.Google Scholar
Maran, S.P., Aller, L.H., Gull, T.R., and Stecher, T.P., 1982, Ap. J. 253, L47.CrossRefGoogle Scholar
Millikan, A.G., 1974, A.J., 79, 1259.Google Scholar
Nussbaumer, J., 1982, Astron. Astroph., 110, L1.Google Scholar
Perinotto, M., Benvenuti, P., and Cacciari, G., 1981, Effects of Mass Loss on Stellar Evolution, ed. Choisi, C., and Stallio, R. (Reidel, Dordrecht), 45.CrossRefGoogle Scholar
Pottasch, S.R., 1981, Physical Processes in Red Giants, ed. Iben, I. and Renzini, A. (Reidel, Dordrecht), 447.CrossRefGoogle Scholar
Reay, N.K., and Worswick, S.P., 1982, MNRAS, 199, 581.CrossRefGoogle Scholar
Rodriguez, L.F., and Moran, J.M., 1982, Nature, 299, 323.CrossRefGoogle Scholar
Shure, M.A., Herter, T., Houck, J.R., Briotta, D.A., Forrest, W.J., Gull, G.E., and McCarthy, J.F., 1982, Preprint.Google Scholar
Stecher, T.P., Maran, S.P., Gull, T.R., Aller, L.H. and Savedoff, M.P., 1982, Preprint.Google Scholar
Terzian, Y., Balick, B., and Bignell, C., 1974, Ap. J., 188, 257.CrossRefGoogle Scholar
Terzian, Y., 1980, Quarterly Journal Roy. Astr. Soc., 21, 81.Google Scholar
Turner, K., and Terzian, Y., 1982, Preprint.Google Scholar