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Planetary Nebulae: Origin and Evolution

Published online by Cambridge University Press:  25 April 2016

D. C. V. Mallik
Affiliation:
Indian Institute of Astrophysics, Bangalore, India

Abstract

There has been a great deal of progress in our understanding of planetary nebulae and their central stars during the past decade and a half. Most of this has come about through progress in observational techniques covering almost the entire electromagnetic spectrum. Theories of planetary nebula evolution have been put to better and better tests as more and more discriminating data have become available.

This review describes some of the progress made in observations and their interpretation, particularly in the context of the evolution of the nebulae and the central stars. It includes a discussion on the improved determinations of magnitudes and temperatures of the central stars, and of progress in the measurement of distances, and a reassessment of the observed mass-distribution of the central stars. The last topic has been at the centre of a lively debate for almost a decade now and has been responsible for a large number of studies of central star evolution, some this review briefly touchs upon.

Type
Invited
Copyright
Copyright © Astronomical Society of Australia 1991

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References

Atherton, P. D., Reay, N. K. and Pottasch, S. R., 1986, Nature, 320, 423.CrossRefGoogle Scholar
Cudworth, K. M., 1974, Astron. J., 79, 1384.CrossRefGoogle Scholar
Daub, C. T., 1982, Astropltys. J., 260, 612.CrossRefGoogle Scholar
Dopita, M. A. and Meatheringham, S. J., 1990, Astropltys. J., 357, 140.CrossRefGoogle Scholar
Downes, R. A., 1986, Astropltys. J. Suppl. Ser., 61, 569.CrossRefGoogle Scholar
Fleming, T. A., Liebert, J. and Green, R. F., 1986, Astrophys. J., 308, 176.CrossRefGoogle Scholar
Gathier, R. and Pottasch, S. R., 1988, Astron. Astrophys., 197, 266.Google Scholar
Gathier, R. and Pottasch, S. R., 1989, Astron. Astrophys., 209, 369.Google Scholar
Heap, S. R. and Augensen, H. J., 1987, Astrophys. J., 313, 268.CrossRefGoogle Scholar
Heap, S. R. and Hintzen, P., 1990, Astrophys. J., 353, 200.CrossRefGoogle Scholar
Iben, I. and Renani, A., 1983, Annu. Rev. Astron. Astrophys., 21, 271.CrossRefGoogle Scholar
Jacoby, G. H. and Kaler, J.B., 1989, Astron. J., 98, 1662.CrossRefGoogle Scholar
Jacoby, G. H., 1988, Astrophys. J., 333, 193.CrossRefGoogle Scholar
Kaler, J.B., 1989, ‘Planetary Nebulae’ in Proc. IAU Symp. No. 131, ed. Torres-Peimbert, S., Kluwer, Dordrecht, p. 229.Google Scholar
Kaler, J. B. and Jacoby, G. H., 1989, Astrophys. J., 345, 871.CrossRefGoogle Scholar
Kaler, J.B. and Jacoby, G. H., 1990, Astrophys. J., in press.Google Scholar
Kaler, J.B., Shaw, R. A. and Kwitter, K.B., 1990, Astrophys. J., in press.Google Scholar
Koester, D., Schulz, H. and Weidemann, V., 1979, Astron. Astrophys., 76, 262.Google Scholar
Lutz, J. H., 1989, ‘Planetary Nebulae’ in Proc. IAU Symp. No. 131, ed. Torres-Peimbert, S., Kluwer, Dordrecht, p. 65.Google Scholar
Maciel, W. J. and Pottasch, S. R., 1980, Astron. Astrophys., 88, 1.Google Scholar
Maliik, D.C.V. and Peimbert, M., 1988, Rev. Mexicana Astron. Astrof., 16, 111.Google Scholar
Pottasch, S. R., 1983, ‘Planetary Nebulae’ in Proc. IAU Symp. No. 103, ed. Flower, D. R., Reidel, Dordrecht, p. 391.Google Scholar
Pottasch, S. R., 1989, ‘Planetary Nebulae’ in Proc. IAU Symp. No. 131, ed. Torres-Peimbert, S., Kluwer, Dordrecht, p. 481.CrossRefGoogle Scholar
Reay, N. K., Pottasch, S. R., Atherton, P. D. and Taylor, K., 1984, Astron. Astrophys., 137, 113.Google Scholar
Renzini, A. and Voli, M., 1981, Astron. Astrophys., 94, 175.Google Scholar
Schonbemer, D., 1981, Astron. Astrophys., 103, 119.Google Scholar
Schonbemer, D. and Weidemann, V., 1983, ‘Planetary Nebulae’ in Proc. IAU Symp. No. 103, ed. Flower, D. R., Reidel, Dordrecht, p. 359.CrossRefGoogle Scholar
Walton, N. A., Reay, N. K., Pottasch, S. R. and Atherton, P. D., 1986, ‘New Insights in Astrophysics’, Proc. Joint NASA/ESA/SERC Conference, ESA SP-263, p. 497.Google Scholar
Walton, N. A., Pottasch, S. R., Reay, N. K. and Taylor, A. R., 1988, Astrophys. J. Lett., 200, L21.Google Scholar
Weidemann, V. and Koester, D., 1983, Astron. Astrophys., 121, 77.Google Scholar
Weidemann, V., 1989, Astron. Astrophys., 213, 155.Google Scholar
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