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- W2079052914 abstract "The luminosity function of planetary nebulae populations in galaxies within 10-15 Mpc distance has a cut-off at bright magnitudes and a functional form that is observed to be invariant in different galaxy morphological types. Thus it is used as a secondary distance indicator in both early and late-type galaxies. Recent deep surveys of planetary nebulae populations in brightest cluster galaxies (BCGs) seem to indicate that their luminosity functions deviate from those observed in the nearby galaxies. We discuss the evidence for such deviations in Virgo, and indicate which physical mechanisms may alter the evolution of a planetary nebula envelope and its central star in the halo of BCGs. We then discuss preliminary results for distances for the Virgo, Hydra I and Coma clusters based on the observed planetary nebulae luminosity functions." @default.
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- W2079052914 date "2012-08-01" @default.
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- W2079052914 title "The planetary nebulae luminosity function and distances to the Virgo, Hydra <scp>i</scp>, and Coma Clusters" @default.
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- W2079052914 doi "https://doi.org/10.1017/s1743921312021564" @default.
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