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Proto-Planetary Nebulae

Published online by Cambridge University Press:  22 September 2016

B. Zuckerman
B. Zuckerman*
Affiliation:
University of Maryland, California Institute of Technology, and University of California at Los Angeles

Extract

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Although rare, planetary nebulae have been extensively studied by astronomers. This affection is certainly due in part to the beauty of the gaseous nebulae but it is also due to the belief that many, probably most, stars of intermediate mass (1–4 M) become planetary nebulae at least once during their lifetimes. If the planetary nebula is an (almost) inevitable stage in stellar evolution, it is important to determine its evolutionary precursors and followers. The latter are likely to be the white dwarfs and the former are generally believed to be red giants. With the advent of infrared and radio techniques it now appears possible, for the first time, to specify the immediate progenitors of planetary nebulae.

Type
Session VII: The Origin of Planetary Nebulaesession VII the Origin of Planetary Nebulae
Information
Symposium - International Astronomical Union , Volume 76: Planetary Nebulae , 1978 , pp. 305 - 313
Copyright
Copyright © Reidel 1978 

References

Abell, G.O. and Goldreich, P.: Publ. Astron. Soc. Pacific, 78, 232.CrossRefGoogle Scholar
Cahn, J.H. and Wyatt, S.P.: 1976, Astrophys. J., 210, 508.Google Scholar
Cohen, M. and Kuhi, L.V.: 1977, Astrophys. J., 213, 79.Google Scholar
Crampton, D., Cowley, A.P., and Humphreys, R.M.: 1975, Astrophys. J., 198, L135.CrossRefGoogle Scholar
Cudworth, K.M.: 1974, Astron. J., 79, 1384.Google Scholar
Evans, N.J. and Beckwith, S.: 1977, Astrophys. J., (in press).Google Scholar
Feast, M.W.: 1968, in Osterbrock, D.E. and O'Dell, C.R. (ed), IAU Symp. #34, Planetary Nebulae, Reidel, Dordrecht, p. 433.Google Scholar
Geballe, T., Wollman, E., and Rank, D.: 1973, Astrophys. J., 183, 499.Google Scholar
Gilmore, W., and Bowers, P.F.: 1977, (private communication).Google Scholar
Goldreich, P.A. and Scoville, N.Z.: 1976, Astrophys. J., 205, 144.CrossRefGoogle Scholar
Härm, R. and Schwarzschild, M.: 1975, Astrophys. J., 200, 324.CrossRefGoogle Scholar
Kuiper, T.B.H., Knapp, G.R., Knapp, S.L., and Brown, R.L.: 1976, Astrophys. J., 204, 408.CrossRefGoogle Scholar
Kwan, J. and Hill, F.: 1977, Astrophys. J., (in press).Google Scholar
Lo, K.Y. and Bechis, K.: 1976, Astrophys. J., 205, L21.CrossRefGoogle Scholar
Lo, K.Y. and Bechis, K.: 1977, (in preparation).Google Scholar
Merrill, K.M. and Stein, W.A.: 1976a, Publ. Astron. Soc. Pacific., 88, 285.Google Scholar
Merrill, K.M. and Stein, W.A.: 1976b, Publ. Astron. Soc. Pacific., 88, 874.Google Scholar
Morris, M.: 1975, Astrophys. J., 197, 603.Google Scholar
Mufson, S.L. and Liszt, H.S.: 1975, Astrophys. J., 202, 183.Google Scholar
Mufson, S.L., Lyon, J., and Marionni, P.A.: 1975, Astrophys. J., 201, L85.CrossRefGoogle Scholar
Ney, E.P., Merrill, K.M., Becklin, E.E., Neugebauer, G., and Wynn-Williams, C.G.: 1975, Astrophys. J., 198, L129.Google Scholar
Osterbrock, D.E.: 1973, in Mem. Soc. Roy. Sci. Liege, 6th Series, 5, 391.Google Scholar
Osterbrock, D.E.: 1974, Astrophysics of Gaseous Nebulae, Freeman, San Francisco, pp 220–222.Google Scholar
Strecker, D.W. and Ney, E.P.: 1974, Astron. J., 79, 797.Google Scholar
Toombs, R.I., Becklin, E.E., Frogel, J.A., Low, S.K., Porter, F.C., and Westphal, J.A.: 1972, Astrophys. J., 173, L71.Google Scholar
Trimble, V., and Sackman, I.J.: 1977, (preprint).Google Scholar
Vanden Bout, P.A. and Lambert, D.: 1976, (private communication).Google Scholar
Vogt, S.S.: 1973, Astron. J., 78, 389.Google Scholar
Westbrook, W.E., Becklin, E.E., Merrill, K.M., Neugebauer, G., Schmidt, M., Wilner, S.P., and Wynn-Williams, C.G.: 1975, Astrophys. J., 202, 407.Google Scholar
Wilson, W.J., Schwartz, P.R., and Epstein, E.E.: 1973, Astrophys. J., 183, 871.Google Scholar
Wood, P.R. and Cahn, J.H.: 1977, Astrophys. J., 211, 499.CrossRefGoogle Scholar
Zuckerman, B., Gilra, D.P., Turner, B.E., Morris, M., and Palmer, P.: 1976, Astrophys. J., 205, L15.CrossRefGoogle Scholar
Zuckerman, B., Palmer, P., Gilra, D.P., Turner, B.E., and Morris, M.: 1977b, Astrophys. J., (submitted).Google Scholar
Zuckerman, B., Palmer, P., Morris, M., Turner, B.E., Gilra, D.P., Bowers, P.F., and Gilmore, W.: 1977a, Astrophys. J., 211, L97.Google Scholar
Zuckerman, B., Silverglate, P., Terzian, Y., and Wolff, M.: 1977c, (in preparation).Google Scholar