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Observations of HII Regions and Planetary Nebulae: the Infrared Emission Bands

Published online by Cambridge University Press:  23 September 2016

Jesse D. Bregman
Jesse D. Bregman*
Affiliation:
NASA Ames Research Center

Abstract

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Advances in infrared spectrometers and the theory that PAHs are responsible for the infrared emission bands have led to a wealth of new information in recent years. High quality data have shown many weak emission bands which are diagnostic of the material producing the bands. While correlations of the strengths of the narrow bands indicate that a single material can account for all of the narrow bands, independent spatial behavior of the narrow and broad components show that they have different origins. Predictions of the behavior of the spectra based on laboratory data have been confirmed observationally, strengthening the theory that PAH molecules are the origin of the infrared emission bands.

Type
Section II: The Overidentified Infrared Emission Features
Information
Symposium - International Astronomical Union , Volume 135: Interstellar Dust , 1989 , pp. 109 - 118
Copyright
Copyright © Kluwer 1989 

References

Aitken, D. K., and Roche, P. F. 1983, M. N. R. A. S., 202, 1233.CrossRefGoogle Scholar
Allamandola, L. J., Tielens, A. G. G. M., and Barker, J. R. 1985, Ap. J. (Letters), 290, L25.CrossRefGoogle Scholar
Allamandola, L. J., Bregman, J. D., Sandford, S. A., Witteborn, F. C., Wooden, D. H., and Rank, D. M. 1988, preprint.Google Scholar
Allamandola, L. J. 1989, in IAU Symposium 135, Interstellar Dust, eds. Allamandola, L. J. and Tielens, A. G. G. M., (Dordrecht: Kluwer), p. 129.CrossRefGoogle Scholar
Barker, J., Allamandola, L. J., and Tielens, A. G. G. M. 1987, Ap. J., 315, L61.CrossRefGoogle Scholar
Bentley, A. 1982, A. J., 87, 1810.CrossRefGoogle Scholar
Bentley, A., Hackwell, J. A., Grasdalen, G. L., and Gehrz, R. D. 1984, Ap. J., 278, 665.Google Scholar
Bregman, J. D. 1977, Pub. A. S. P., 89, 335.CrossRefGoogle Scholar
Bregman, J. D., and Rank, D. M. 1975, Ap. J. (Letters), 195, L125.CrossRefGoogle Scholar
Bregman, J. D., Dinerstein, H. L., Goebel, J. H., Lester, D. F., Witteborn, F. C., and Rank, D. M. 1983, Ap. J., 274, 666.CrossRefGoogle Scholar
Bregman, J. D., Allamandola, L. J., Tielens, A. G. G. M., Witteborn, F. C., Rank, D. M., and Wooden, D. H. 1987, in Summer School on Interstellar Processes, Abstracts of Contributed Papers, eds. Hollenbach, D. and Thronson, H., (NASA TM 88342), p. 117.Google Scholar
Bregman, J. D., Allamandola, L. J., Tielens, A. G. G. M., Geballe, T., and Witteborn, F. C. 1988, Ap. J., submitted.Google Scholar
Cohen, M., Tielens, A. G. G. M., and Allamandola, L. J. 1985, Ap. J. (Letters), 299, L93.CrossRefGoogle Scholar
Cohen, M., Allamandola, L. J., Tielens, A. G. G. M., Bregman, J. D., Simpson, J. P., Witteborn, F. C., Wooden, D. H., and Rank, D. 1986, Ap. J., 302, 737.CrossRefGoogle Scholar
Cohen, M., Tielens, A. G. G. M., Bregman, J. D., Witteborn, F. C., Rank, D. M., Allamandola, L. J., Wooden, D. H., and de Muizon, M. 1988, Ap. J., submitted.Google Scholar
de Muizon, M., Geballe, T. R., d'Hendecourt, L. B., and Baas, F. 1986, Ap. J. (Letters), 306, L105.CrossRefGoogle Scholar
Duley, W. W., and Williams, D. A. 1981, M. N. R. A. S., 196, 269.CrossRefGoogle Scholar
Geballe, T. R., Lacy, J. H., Persson, S. E., McGregor, P. J., and Soifer, B. T. 1985, Ap. J., 292, 500.CrossRefGoogle Scholar
Geballe, T. R., Tielens, A. G. G. M., Allamandola, L. J., Morehouse, A., and Brand, P. W. J. L. 1988, Ap. J., in press.Google Scholar
Gillett, F. C., Forrest, W. J., and Merrill, K. M. 1973, Ap. J., 183, 87.Google Scholar
Goebel, J. H., Rank, D. M., and Cohen, M. 1987, in Infrared Astronomy with Arrays, eds. Wynn-Williams, C. G., and Becklin, E. E., (Honolulu: University of Hawaii), p. 305.Google Scholar
Léger, A. and d'Hendecourt, L. B. 1987, in Polycyclic Aromatic Hydrocarbons and Astrophysics, eds. Léger, A., d'Hendecourt, L. B., and Boccara, N., (Dordrecht: Reidel), p. 223.Google Scholar
Léger, A., and Puget, J. L. 1984, Astr. Av., 137, L5.Google Scholar
Roche, P., Aitken, D. A., and Smith, C. H. 1988, preprint.Google Scholar
Russell, R. W., Soifer, B. T., and Willner, S. P. 1977, Ap. J. (Letters), 217, L149.CrossRefGoogle Scholar
Sandford, S. A., Witteborn, F. C., Bregman, J. D., Cohen, M., and Allamandola, L. J. 1988, BAAS, 19, 952.Google Scholar
Sellgren, K. 1981, Ap. J., 245, 138.CrossRefGoogle Scholar
Sellgren, K. 1984, Ap. J., 277, 623.CrossRefGoogle Scholar
Tokunaga, A. T., and Young, E. T. 1980, Ap. J. (Letters), 237, L149.Google Scholar
Tokunaga, A. T., Nagata, T., Sellgren, K., Smith, R. G., Onaka, T., Nakada, Y., Sakata, A., and Wada, S. 1988, Ap. J., 328, 709.CrossRefGoogle Scholar
Tresch-Fienberg, R. 1985, , .Google Scholar
Witteborn, F. C., Sandford, S. A., Bregman, J. D., Allamandola, L. J., Wooden, D. H., Cohen, M., Graps, A. L. 1989a, Ap. J. in press.Google Scholar
Witteborn, et al. 1989b, in Interstellar Dust Contributed Papers, eds. Tielens, A. G. G. M. and Allamandola, L. J., NASA CP-3036.Google Scholar