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Multiple Shell Planetary Nebulae

Published online by Cambridge University Press:  19 July 2016

You-Hua Chu
You-Hua Chu*
Affiliation:
Astronomy Department, University of Illinois, 1011 W. Springfield Avenue, Urbana, IL 61801, U. S. A.

Abstract

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It has been shown in several independent investigations that the multiple-shell phenomenon is prevalent in planetary nebulae. Despite the common classification, the multiple shell planetary nebulae are a heterogeneous group of objects, as testified by the wide variety of their morphologies and physical structures. There are two types of double-shell structures that are seen frequently: one has an inner shell expanding supersonically into a faint, subsonically expanding halo, and the other has a bright attached envelope co-expanding with the inner shell. The physical structures and relative elemental abundances in the shells are reviewed, and their possible formation mechanisms are discussed.

Type
II. Nebular Properties
Information
Symposium - International Astronomical Union , Volume 131: Planetary Nebulae , 1989 , pp. 105 - 116
Copyright
Copyright © Kluwer 1989 

References

Aller, L. H., Keyes, C. D., and Feibelman, W. A. 1986, Ap. J., 311. 930.Google Scholar
Balick, B. 1987a, A. J., 94, 671.CrossRefGoogle Scholar
Balick, B. 1987b, this volume.Google Scholar
Balick, B., Preston, H., and Vicke, V. 1988, submitted to A. J.Google Scholar
Barker, T. 1983, Ap. J., 267, 630.Google Scholar
Barker, T. 1985, Ap. J., 294, 193.Google Scholar
Barker, T. 1986, Ap. J., 308, 314.Google Scholar
Bässgen, M., Bässgen, G., Barnstedt, J., Grewing, M., and Bianchi, L. 1986, Mitt. Astr. Ges., Nr. 67, p. 342.Google Scholar
Bässgen, M., Bässgen, G., Grewing, M., Cerrato, S., and Bianchi, L. 1987, in this volume.Google Scholar
Cerruti-Sola, M., and Perinotto, M. 1985, Ap. J., 291, 237.Google Scholar
Chu, Y.-H., and Jacoby, G. H. 1987, in this volume.Google Scholar
Chu, Y.-H., and Jacoby, G. H. 1988, in preparation.Google Scholar
Chu, Y.-H., Jacoby, G. H., and Arendt, R. 1987, Ap. J. Suppl., 64, 529.Google Scholar
Cohen, M., Harrington, J. P., and Hess, R. 1984, Ap. J., 283, 687.Google Scholar
Curtis, H. D. 1918, Pub. Lick Obs., 13, 57.Google Scholar
Duncan, J. C. 1987, Ap. J., 86, 496.Google Scholar
Gieseking, F., Becker, I., and Solf, J. 1985, Ap. J. (Letters), 295, L17.Google Scholar
Gieseking, F., and Solf, J. 1986, Astr. Ap., 163, 174.Google Scholar
Hippelein, H. H., Bässgen, M., and Grewing, M. 1985, Astr. Ap., 152, 213.Google Scholar
Iben, I. Jr., Kaler, J. B., Truran, J. W., and Renzini, A. 1983, Ap. J., 264, 605.Google Scholar
Iben, I. Jr., and Tutukov, A. V. 1987, in this volume.Google Scholar
Jacoby, G. H., and Chu, Y.-H. 1987, in this volume.Google Scholar
Jacoby, G. H., and Ford, H. C. 1983, AP. J., 266, 298.Google Scholar
Jacoby, G. H., Quigley, R. J., and Africano, J. L. 1987, Pub. A. S. P., 99, 672.Google Scholar
Jewitt, D. C., Danielson, G. E., and Kupferman, P. N. 1986, Ap. J., 302. 727.Google Scholar
Kaler, J. B. 1974, A. J., 79, 594.Google Scholar
Kwok, S. 1983, in IAU Symp. No. 103, “Planetary Nebulae”, ed. Flower, D. R., (Reidel: Dordrecht), p. 293.CrossRefGoogle Scholar
Kwok, S. 1987, in “Late Stages of Stellar Evolution”, eds. Kwok, S. and Pottasch, S., (Reidel: Dordrecht), p. 321.Google Scholar
Lutz, J., Lame, N. J., and Balick, B. 1987, in this volume.Google Scholar
Manchado, A., Pottasch, S. R., and Mampaso, A. 1987a, in this volume.Google Scholar
Manchado, A., Pottasch, S. R., and Mampaso, A. 1987b, in this volume.Google Scholar
Mathews, W. G. 1978, in IAU Symp. No. 76, “Planetary Nebulae”, ed. Terzian, Y. (Reidel: Dordrecht), p. 251.Google Scholar
Middlemass, D., Clegg, R. E. S., and Walsh, J. R. 1987, in this volume.Google Scholar
Millikan, A. G. 1974, A. J., 79, 1259.Google Scholar
Minkowski, R., and Osterbrock, D. 1960, Ap. J., 131, 537.Google Scholar
Moreno, M. A., and López, J. A. 1987, Astr. Ap., 178, 319.Google Scholar
O'Dell, C. R., and Ball, M. E. 1985, Ap. J., 289, 526.Google Scholar
Perek, L., and Kohoutek, L. 1987, Catalogue of Galactic Planetary Nebulae (Prague: Czechoslovaak Academy of Science)Google Scholar
Pismis, P., and Moreno, M. A. 1987, in this volume.Google Scholar
Reay, N. K., Atherton, P. D., and Taylor, K. 1983a, M. N. R. A. S., 203, 1079.Google Scholar
Reay, N. K., Atherton, P. D., and Taylor, K. 1983b, M. N. R. A. S., 203, 1087.Google Scholar
Rosado, M. 1986, Rev. Mexicana. Astr. Ap., 13, 49.Google Scholar
Ruiz, M. T., Heathcote, S. R., and Weller, W. G. 1987, in this volume.Google Scholar
Sabbadin, F. 1984, Astr. Ap. Suppl., 58, 273.Google Scholar
Schmidt-Voigt, M., and Köppen, J. 1987a, Astr. Ap., 174, 211.Google Scholar
Schmidt-Voigt, M., and Köppen, J. 1987b, Astr. Ap., 174, 223.Google Scholar
Walsh, J. R., and Meaburn, J. 1987, M. N. R. A. S., 224, 885.Google Scholar
Webster, B. L. 1978, M. N. R. A. S., 185, 45p.Google Scholar
Weller, W. G., and Heathcote, S. R. 1987a, in “Late Stages of Stellar Evolution”, eds. Kwok, S. and Pottasch, S. R., (Reidel: Dordrecht), p. 409.Google Scholar
Weller, W. G., and Heathcote, S. R. 1987b, in this volume.Google Scholar
Welty, D. E. 1983, Pub. A. S. P., 95, 217.Google Scholar