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Physical Characteristics of Ionized Gaseous Nebulae*

Published online by Cambridge University Press:  15 February 2018

Donald E. Osterbrock
Donald E. Osterbrock*
Affiliation:
Lick Observatory, Board of Studies in Astronomy & AstrophysicsUniversity of California, Santa Cruz

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The chief advantages of the Space Telescope over conventional ground-based telescopes, namely, ability to observe ultraviolet radiation and high angular resolution, make it particularly valuable for research on gaseous nebulae. These objects are interesting not only in themselves, but also because they provide an opportunity to measure the abundances of the common light elements in the first two rows of the periodic table. H II regions are samples of interstellar matter from which stars are now forming in our galaxy, and in other galaxies. Planetary nebulae are objects approaching the end of their evolution as luminous stars, in which an outer shell has been thrown off and is returning to interstellar space. They represent one of the most prolific sources of mass return to interstellar matter at the present time in our galaxy.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 54: Scientific Research with the Space Telescope , 1979 , pp. 99 - 121
Copyright
Copyright © Marshall Space Flight Center 1979

Footnotes

*

Contributions from the Lick Observatory, No. 420

References

Aller, L. H.: 1979, P.A.S.P. 88, 574.Google Scholar
Alloin, D., Collin-Souffrin, S. and Joly, M.: 1979, Astron. Astrophysics Supple. 37. 361.Google Scholar
Bahcall, J. N. and O'Dell, C. R.: 1979, This Conference.Google Scholar
Balick, B. and Sneden, C.: 1979, Ap.J. 208, 336.Google Scholar
Barker, T.: 1978a, Ap.J. 219, 914.Google Scholar
Barker, T.: 1978b, Ap.J. 220, 193.Google Scholar
Bely, O.: 1966, Proc. Phys. Soc. Lon. A. 88, 587.Google Scholar
Bohlin, R. C., Marionni, P. A. and Stecker, T. P.: 1975, Ap.J. 202, 415.Google Scholar
Bohlin, R. C, Harrington, J. P. and Stecker, T. P.: 1978, Ap.J. 219, 575.Google Scholar
Burke, P. B. and Moores, D. L.: 1968, J.Phys. B. 1, 575.Google Scholar
Butler, S. E., Bender, C. F. and Dalgarno, A.: 1979, Ap.J. 230, L59.Google Scholar
Chevalier, R.: 1977, Ann. Rev. Astron. Ap. 15, 175.Google Scholar
Danziger, I. J. and Dennefeld, M. : 1979, P.A.S.P. 88, 44.Google Scholar
Dopita, M. A.: 1977, Ap.J. Supp. 33, 437.Google Scholar
Dopita, M. A., Isobe, S. and Meaburn, J.: 1975, Ap. Space Sci. 34, 91.Google Scholar
Flower, D. R. and Launay, J. M.: 1973, Astron. Ap. 29, 321.Google Scholar
Flower, D. R. and Nussbaumer, H.: 1975, Astron. Ap. 42, 265.Google Scholar
Flower, D. R., Nussbaumer, H. and Shild, H.: 1979, Astron. Ap. 72, Ll.Google Scholar
Giles, K.: 1979, M.N.R.A.S. 198, 47P.Google Scholar
Grewing, M., Boksenberg, A., Seaton, M. J., Snijders, M.A.J., Wilson, R., Boggess, A., Bohlin, R. C., Perry, P. M., Shiffer, I.H., Gondhalekar, P. M., Macchetto, F., Savage, B. D., Jenkins, E. G., Johnson, H. M., Perionotto, M. and Whittet, D. C. B.: 1978, Nature 275, 394.Google Scholar
Hawley, S. A.: 1978, Ap.J. 224, 417.Google Scholar
Hawley, S. A. and Grandi, S. A.: 1977, Ap.J. 217, 420.Google Scholar
Hawley, S. A. and Miller, J. S.: 1977, Ap.J. 212, 94.Google Scholar
Jackson, A. R. G.: 1973, M.N.R.A.S. 165, 53.Google Scholar
Kaler, J. B.: 1979, Ap.J. Supp. 31, 517.Google Scholar
Laques, P. and Vidal, J. L.: 1979, Astron. Ap. 73, 97.Google Scholar
Longair, M. S.: 1979, Q.J.R.A.S. 20, 5.Google Scholar
Lutz, J. H. and Seaton, M. J.: 1979, M.N.R.A.S. 187, 1P.Google Scholar
Malinovsky, M.: 1975, Astron. Ap. 43, 101.Google Scholar
Miller, J.S.: 1974, Ann. Rev. Astron. Ap. 12, 331.Google Scholar
Minkowski, R.: 1968, in Osterbrock, D. E. and O'Dell, C. R. (ed)., D., Planetary Nebulae Reidel Co., Dordrecht, p. 465.Google Scholar
Mufson, S., Lyon, J. and Marionni, R. A.: 1975, Ap.J. 201, L85.Google Scholar
O'Dell, C. R. : 1962, Ap.J. 135, 371.Google Scholar
Osterbrock, D. E.: 1963, Planetary Space Sci. 11, 621.Google Scholar
Osterbrock, D. E.: 1970, Ap.J. 160, 25.Google Scholar
Osterbrock, D. E.: 1974, Astrophysics of Gaseous Nebulae, W. H. Freeman & Co. , San Francisco.Google Scholar
Osterbrock, D. E. and Wallace, R. K.: 1977, Ap. Lett. 19, 11.Google Scholar
Peimbert, M. and Torres-Peimbert, S.: 1977, M.N.R.A.S. 179, 217.Google Scholar
Peimbert, M., Torres-Peimbert, S. and Rayo, J. F.: 1978, Ap.J. 220, 516.Google Scholar
Pottasch, S. R. , Wesselius, P. R. and van Duinen, R. J.: 1978a, Astron. Ap. 70, 629.Google Scholar
Pottasch, S. R. , Wesselius, P. R. , Wu, C.-C, Fierten, F. J. and van Duinen, R. J.: 1978b, Astron. Ap. 62, 95.Google Scholar
Pradhan, A.K.: 1974, J. Phys. B. 7, L509.Google Scholar
Raymond, J.C.: 1979, Ap.J. Supp. 39, 1.Google Scholar
Reay, N. K. and Worswick, S. P.: 1979, Astron. Ap. 72, 31.Google Scholar
Salpeter, E. E.: 1977, Ann. Rev. Astron. Ap. 15, 267.Google Scholar
Scott, P. F.: 1973, M.N.R.A.S. 161, 35P.Google Scholar
Seaton, M. H.: 1975, M.N.R.A.S. 170, 475.Google Scholar
Seaton, M. J.: 1979, M.N.R.A.S. 187, 785.Google Scholar
Shemansky, D. E., Sandel, B. R. and Broadfoot, A. L.: 1979, Ap. J. in press.Google Scholar
Shields, G. A.: 1978, Ap.J. 219, 565.Google Scholar
Spitzer, L.: 1978, Physical Processes in the Interstellar Medium, John Wiley & Sons, New York.Google Scholar
Torres-Peimbert, S. and Peimbert, M.: 1977, Rev. Mexicana Astron. A. 2, 181.Google Scholar
Treffers, R. R., Fink, U., Larson, H. P. and Gautier, T. N.: 1979, Ap.J. 209, 793.Google Scholar
Van Wyngaarden, W. L. and Henry, R. J. W.: 1979, J. Phys. B. 9, 1461.Google Scholar
Woodgate, B. E., Kirshner, R. P. and Balon, R. J. 1977, Ap.J. 218, L129.Google Scholar