Hostname: page-component-78c5997874-xbtfd Total loading time: 0 Render date: 2024-11-14T23:41:50.219Z Has data issue: false hasContentIssue false

Why are Planetary Nebulae Poor Distance Indicators?

Published online by Cambridge University Press:  07 August 2017

G.A. Tammann*
Affiliation:
Astronomisches Institut der Universität Basel, Venusstraße 7, CH-4102 Binningen

Abstract

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.

It is shown from multiple evidence that the λ 5007 Å luminosity of the brightest shells of planetary nebulae has intrinsic scatter, which is well approximated for the brightest objects by an exponential luminosity function, as proposed by Bottinelli et al. (1991). The resulting open-ended luminosity function weakens the usefulness of planetary nebulae as distance indicators.

Type
VI. Planetary Nebulae in Galactic Systems
Copyright
Copyright © Kluwer 1993 

References

Bottinelli, L., Gouguenheim, L., Paturel, G., and Teerikorpi, P. 1991, A.A. 252, 550.Google Scholar
Ciardullo, R., and Jacoby, G.H. 1992, Ap. J., in press.Google Scholar
Ciardullo, R., Jacoby, G.H., and Ford, H.C. 1989b, Ap. J. 344, 715.CrossRefGoogle Scholar
Ciardullo, R., Jacoby, G.H., Ford, H.C., and Neill, J.D. 1989a, Ap. J. 339, 53.CrossRefGoogle Scholar
Ciardullo, R., Jacoby, G.H., and Harris, W.E. 1991, Ap. J. 383, 487.CrossRefGoogle Scholar
Dopita, M.A., Jacoby, G.H., and Vassiliadis, E. 1992, Ap. J. 389, 27.CrossRefGoogle Scholar
Faber, S.M., Wegner, G., Burstein, D., Davies, R.L., Dressier, A., Lynden-Bell, D., and Terlevich, R.J. 1989, Ap. J. Suppl. 69, 763.CrossRefGoogle Scholar
Ferguson, H.C., and Davidsen, A.F. 1992, preprint.Google Scholar
Harris, W.E. 1990, P.A.S.P. 102, 966.CrossRefGoogle Scholar
Jacoby, G.H. 1969, Ap. J. 339, 39.CrossRefGoogle Scholar
Jacoby, G.H. et al. 1992, P.A.S.P. 104, 599.CrossRefGoogle Scholar
Jacoby, G.H., Ciardullo, R., and Ford, H.C. 1990a, Ap. J. 356, 332.CrossRefGoogle Scholar
Jacoby, G.H., Walker, A.R., and Ciardullo, R. 1990b, Ap. J. 365, 471.CrossRefGoogle Scholar
Jacoby, G.H., Ciardullo, R., Ford, H.C., and Booth, J. 1989, Ap. J. 344, 704.CrossRefGoogle Scholar
Jacoby, G.H., Walker, A.R., and Ciardullo, R. 1990, Ap. J. 365, 471.CrossRefGoogle Scholar
Madore, B.F., and Freedman, W.L. 1991, P.A.S.P. 103, 933.CrossRefGoogle Scholar
Sandage, A., and Carlson, G. 1988, A.J. 96, 1599.CrossRefGoogle Scholar
Sandage, A., Saha, A., Tammann, G.A., Panagia, N., and Macchetto, F. 1993, Ap. J. Letters, in press.Google Scholar
Sandage, A., and Tammann, G.A. 1974a, Ap. J. 194, 559.CrossRefGoogle Scholar
Sandage, A., and Tammann, G.A. 1974b, Ap. J. 191, 603.CrossRefGoogle Scholar
Schmidt, B.P., Kirshner, R.P., and Eastman, R.G. 1992, Ap. J., in press.Google Scholar
Tammann, G.A. 1992, Physica Scripta T 43, 31.CrossRefGoogle Scholar
Tonry, J.L. 1991, Ap. J. Letters 373, L1.CrossRefGoogle Scholar