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Infrared Emission Lines in Planetary Nebulae

Published online by Cambridge University Press:  18 September 2017

Harriet L. Dinerstein
Harriet L. Dinerstein*
Affiliation:
NASA Ames Research Center, Moffett Field, California 94035

Abstract

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Advances in infrared spectroscopy have led to the detection of many forbidden fine-structure emission lines in planetary nebulae. Measurements of these lines offer sensitive probes of the physical conditions and ionization structure, and lead to improved abundance determinations. This paper reviews recent observations and discusses the ways in which infrared line measurements can contribute to our knowledge of planetary nebulae.

Type
Section I: Observations of Planetary Nebulae
Information
Symposium - International Astronomical Union , Volume 103: Planetary Nebulae , 1983 , pp. 79 - 88
Copyright
Copyright © Reidel 1983 

References

Aitken, D. K., Roche, P. F., Spenser, P. M., and Jones, B.: 1979, Ap. J. 233, 925.Google Scholar
Aller, L. H.: 1978, in “Planetary Nebulae,” IAU Symposium No. 76, Terzian, Y. (ed.), Dordrecht: Reidel, pp. 225–234.Google Scholar
Aller, L. H. and Epps, H. W.: 1976, Ap. J. 204, 445.Google Scholar
Barker, T.: 1978a, Ap. J. 220, 193.Google Scholar
Barker, T.: 1978b, Ap. J. 221, 145.Google Scholar
Barker, T.: 1979, Ap. J. 227, 863.Google Scholar
Beck, S. C., Lacy, J. H., Townes, C. H., Aller, L. H., Geballe, T. R., and Baas, F.: 1981, Ap. J. 249, 592.Google Scholar
Beckwith, S., Evans, N. J. II, Natta, A., Russell, R. W., and Wyant, J.: 1982, in preparation.Google Scholar
Bohuski, T. J., Dufour, R. J., and Osterbrock, D. E.: 1974, Ap. J. 188, 529.Google Scholar
Bregman, J. D.: 1978, Pub. Astron. Soc. Pac. 90, 548.Google Scholar
Bregman, J. D., Dinerstein, H. L., Goebel, J. H., Lester, D. F., Witteborn, F. C., and Rank, D. M.: 1981, Bull. Am. Astron. Soc. 13, 852.Google Scholar
Dinerstein, H. L.: 1980a, Ap. J. 237, 486.Google Scholar
Dinerstein, H. L.: 1980b, , University of California, Santa Cruz.Google Scholar
Dinerstein, H. L. and Rank, D. M.: 1982, in preparation.Google Scholar
Dinerstein, H. L., Lester, D. F., Bregman, J. D., Witteborn, F. C., and Rank, D. M.: 1982, in preparation.Google Scholar
Eissner, W. and Seaton, M. J.: 1974, J. Phys. B: Atom. Molec. Phys. 7, 2533.Google Scholar
Forrest, W. J., McCarthy, J. F., and Houck, J. R.: 1980, Ap. J. Lett. 240, L37.Google Scholar
Garstang, R. H.: 1968, in “Planetary Nebulae,” IAU Symposium No. 34, Osterbrock, D. E. and O'Dell, C. R. (eds.), Dordrecht: Reidel, pp. 143–152.Google Scholar
Garstang, R. H., Robb, W. D., and Rountree, S. P.: 1978, Ap. J. 222, 384.Google Scholar
Grasdalen, G.: 1979, Ap. J. 229, 587.Google Scholar
Greenberg, L. T., Dyal, P., and Geballe, T. R.: 1977, Ap. J. Lett. 213, L71.Google Scholar
Kaler, J. B.: 1978, Ap. J. 225, 527.Google Scholar
Kaler, J. B.: 1979, Ap. J. 228, 163.Google Scholar
Kaler, J. B.: 1980, Ap. J. 239, 78.Google Scholar
McCarthy, J. F.: 1979, , Cornell University.Google Scholar
Melnick, G., Russell, R. W., Gull, G. E., and Harwit, M.: 1981, Ap. J. 243, 170.Google Scholar
Moseley, H.: 1982, private communication.Google Scholar
Natta, A., Panagia, N., and Preite-Martinez, A.: 1980, Ap. J. 242, 596.Google Scholar
Olthof, H. and Pottasch, S. R.: 1975, Astr. Ap. 43, 291.Google Scholar
Osterbrock, D. E.: 1974, “Astrophysics of Gaseous Nebulae,” San Francisco: Freeman.Google Scholar
Pagel, B. E. J.: 1978, Mon. Not. Roy. Astron. Soc. 183, 1 p.Google Scholar
Peimbert, M.: 1967, Ap. J. 150, 825.Google Scholar
Peimbert, M.: 1978, in “Planetary Nebulae,” IAU Symposium No. 76, Terzian, Y. (ed.), Dordrecht: Reidel, pp. 215–224.Google Scholar
Peimbert, M. and Costero, R.: 1969, Bol. Obs. Tonant. y Tacu. 5, 3.Google Scholar
Peimbert, M. and Torres-Peimbert, S.: 1971, Ap. J. 168, 413.Google Scholar
Petrosian, V.: 1970, Ap. J. 159, 833.Google Scholar
Rank, D. M.: 1978, in “Planetary Nebulae,” IAU Symposium No. 76, Terzian, Y. (ed.), Dordrecht: Reidel, pp. 103–110.Google Scholar
Roche, P. F.: 1982, , University College, London.Google Scholar
Rubin, R.: 1969, Ap. J. 155, 841.Google Scholar
Russell, R. W., Soifer, B. T., and Willner, S. P.: 1977, Ap. J. Lett. 217, L149.Google Scholar
Saraph, H. E., Seaton, M. J., and Shemming, J.: 1969, Phil. Trans. Roy. Soc. London, Ser. A 264, 77.Google Scholar
Shields, G. A., Aller, L. H., Keyes, C. D., and Czyzak, S. J.: 1981, Ap. J. 248, 569.Google Scholar
Simpson, J. P.: 1975, Astron. Ap. 39, 43.Google Scholar
Soifer, B. T. and Pipher, J. L.: 1978, Ann. Rev. Astron. Ap. 16, 335.Google Scholar
Storey, J. W. V., Watson, D. M., and Townes, C. H.: 1980, Int. J. Infr. Millim. Waves 1, 15.Google Scholar
Torres-Peimbert, S. and Peimbert, M.: 1977, Rev. Mex. Astron. Ap. 2, 181.Google Scholar
Watson, D. M. and Storey, J. W. V.: 1980, Int. J. Infr. Millim. Waves 1, 609.Google Scholar
Watson, D. M., Storey, J. W. V., Townes, C. H., and Haller, E. E.: 1981, Ap. J. 250, 605.Google Scholar
Willner, S. P., Jones, B., Puetter, R. C., Russell, R. W., and Soifer, B. T.: 1979, Ap. J. 234, 496.Google Scholar