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Planetary Nebulae and the Cosmic Distance Scale
Published online by Cambridge University Press: 30 March 2016
Abstract
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Planetary nebula luminosity functions provide very accurate distances to galaxies as judged by comparisons with other techniques, including Cepheids; systematic effects cannot be significant. The method is empirical and is a consequence of the shallow initial-final mass relationship predicted by stellar evolution and directly measured. From distances to ∼ 30 galaxies, the PNLF yields H0 = 79, in excellent agreement with recent Cepheid discoveries in Virgo.
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- II. Joint Discussions
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- Copyright © Kluwer 1995
References
Jacoby, G.H., & Ciardullo, R.
1992, in IAU Symposium 155: Planetary Nebulae (Dordrecht: Reidel), ed. Weinberger, R. & Acker, A., p. 503.Google Scholar
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1988, in The Extragalactic Distance Scale, A.S.P. Conference Series No. 4, ed. van den Bergh, S. & Pritchet, C.J. (Provo: Brigham Young University Press), p.42.Google Scholar
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