Hostname: page-component-586b7cd67f-gb8f7 Total loading time: 0 Render date: 2024-11-29T15:18:23.939Z Has data issue: false hasContentIssue false
  • English
  • Français

Distances of Planetary Nebulae

Published online by Cambridge University Press:  07 August 2017

Yervant Terzian
Yervant Terzian*
Affiliation:
Cornell University, NAIC, Ithaca, New York

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

One of the most fundamental physical parameter in astronomy is the distance to the objects we detect in the universe. For many classes of astronomical objects, accurate and proven methods have been developed to determine their distances. Such classes of objects include stars within ∼100 pc from the sun, binary stellar systems, variable stars, stellar clusters, main sequence stars, and other galaxies. It has been, however, more difficult to develop satisfactory methods to determine accurate distances to the more than 1000 planetary nebulae that have been discovered in our galaxy.

Type
III. Highlights on the Nebulae
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 109 - 121
Copyright
Copyright © Kluwer 1993 

References

Acker, A., 1978, Astron. Astrophys. Suppl., 33, 367.Google Scholar
Aller, L. H., 1991 Asteroids to Quasars, ed. Lugger, P. M., (Cambridge University Press), 85.Google Scholar
Amnuel, P. R., Guseinov, O. H., Novruzova, H. I., and Rustamov, Yu. S., 1984, Astrophys. Space Sc., 107, 19.CrossRefGoogle Scholar
Anguita, C., Gutterrez-Moreno, A., and Moreno, H., 1992, This Symposium, Contr. Paper.Google Scholar
Bottinelli, L., Gouguenheim, L., Paturel, G., and Teerikorpi, P., 1991, Astron. Astrophys., 252, 550.Google Scholar
Cahn, J. H., and Kaler, J. B., 1971, Astrophys. J. Suppl., 22, 319.Google Scholar
Cahn, J. H., 1976, Astron. J., 81, 407.Google Scholar
Cahn, J. H., Kaler, J. B., and Stanghellini, L., 1992, Astron. Astrophys. Suppl., (in press).Google Scholar
Clegg, R. E. S., Hoare, M. G., and Walsh, J. R., 1989, Planetary Nebulae, ed. Torres-Peimbert, S., (Kluwer Academic Publ.), 443.Google Scholar
Cudworth, K. M., 1974, Astron. J., 79, 1384.CrossRefGoogle Scholar
Daub, C. T., 1982, Astrophys. J., 260, 612.Google Scholar
Davis, L. E., Seaquist, E. R., and Purton, C. R., 1979, Astrophys. J., 230, 434.Google Scholar
Feast, M., 1987, The Galaxy, eds., Gilmore, G. and Craswell, B., (D. Reidel Publ. Co.).Google Scholar
Ford, H. C., Ciardullo, R., Jacoby, G. H., and Hui, X., 1989, Planetary Nebulae, ed. Torres-Peimbert, S., (Kluwer Academic Publ.), 335.Google Scholar
Gathier, R., 1987, Astron. Astrophys. Suppl., 71, 245.Google Scholar
Ishida, K., and Weinberger, R., 1987, Astron. Astrophys., 178, 227.Google Scholar
Jacoby, G. H., 1989, Astrophys. J., 339, 39.Google Scholar
Jacoby, G. H., Ciardullo, R., and Ford, H. C., 1990, Astrophys. J., 356, 332.Google Scholar
Knapp, G. R., and Morris, M., 1985, Astrophys. J., 292, 640.Google Scholar
Liller, M. H., and Liller, W., 1968, Planetary Nebulae, eds. Osterbrock, D. and O'Dell, C. R., (D. Reidel Publ. Co.), 38.Google Scholar
Liller, W., 1978, Planetary Nebulae, ed. Terzian, Y., (D. Reidel Publ. Co.), 35.Google Scholar
Lutz, J. H., 1989, Planetary Nebulae, ed. Torres-Peimbert, S., (Kluwer Academic Publ.), 65.Google Scholar
Maciel, W. J., and Pottasch, S. R., 1980, Astron. Astrophys., 88, 1.Google Scholar
Maciel, W. J., 1985, Rev. Mexicana Astron. Astrof., 10, 199.Google Scholar
Mallik, D. C. V., and Peimbert, M., 1988, Rev. Mexicana Astron. Astrof., 16, 111.Google Scholar
Masson, C. R., 1986, Astrophys. J., 302, L27.Google Scholar
Masson, C. R., 1989, Astrophv. J., 346, 243.Google Scholar
Milne, D. K. and Aller, L. H., 1975, Astron. Astrophys., 38, 183.Google Scholar
Phillips, J. P., 1989, Planetary Nebulae, ed. Torres-Peimbert, S. (Kluwer Academic Publ.), 425.Google Scholar
Pier, J. R., Harris, H. C., Dahn, C. C. and Monet, D. G., 1992, This Symposium, Contr. Paper.Google Scholar
Pottasch, S. R., 1980, Astron. Astrophys., 89, 336.Google Scholar
Pottasch, S. R., Goss, W. M., Arnal, E. M., and Gathier, R., 1982, Astron. Astrophys., 106, 229.Google Scholar
Pottasch, S. R., 1990, Astron. Astrophys., 236, 231.Google Scholar
Pottasch, S. R., and Zijlstra, A. A., 1992, Astron. Astrophys., 256, 251.Google Scholar
Puche, D., et. al., 1988, Astron. Astrophys., 206, 89.Google Scholar
Rood, R. T., Bania, T. M., and Wilson, T. L., 1992, Nature, 355, 618.Google Scholar
Seaquist, E. R., 1991, Astron. J., 101, 2141.Google Scholar
Stasińska, G., Tylenda, R., Acker, A., and Stenholm, B., 1991, Astron. Astrophys., 247, 173.Google Scholar
Terzian, Y., 1980, Q. Jl. R. Astro. Soc., 21, 82.Google Scholar
Terzian, Y., 1987, Sky and Telescope, 73, 128.Google Scholar
Terzian, Y., Hajian, A., Bignell, C., and Phillips, J. A., 1992, (preprint).Google Scholar
Tweedy, R. W., and Napiwotzki, R., 1992, Monthly Notices R.A.S. (in press).Google Scholar
Zhang, C. Y., and Kwok, S., 1992, Astron. Astrophys. Suppl., (submitted).Google Scholar