Post-AGB Stars as Standard Extragalactic Candles

dc.creatorBond, Howard E.
dc.date1997-02-01
dc.date.accessioned2026-07-07T02:22:51Z
dc.date.available2026-07-07T02:22:51Z
dc.descriptionStars evolving off the asymptotic giant branch and passing through spectral types F and A are excellent candidates for a new extragalactic candle. These post-AGB (PAGB) stars are the brightest members of Population II systems. They should have a narrow luminosity function, bounded from above by the shorter transition times of more massive and more luminous remnants, and from below by the core mass corresponding to the lowest-mass stars that are leaving the main sequence. Moreover, PAGB A-F supergiants are easily recognized because of their enormous Balmer jumps, and should lie both in ellipticals and the halos of spirals. I describe a photometric system that combines Gunn u with the standard BVI bandpasses, and report a successful search for PAGB stars in the halo of M31 using this uBVI system. The zero-point calibration will come from PAGB A and F stars in Galactic globular clusters. Four are presently known, and have a mean Mv = -3.4 with a scatter of only 0.2 mag. With this Mv we exactly reproduce the accepted M31 distance from its halo PAGB stars. Future plans include a uBVI survey of Milky Way globular clusters and Local Group galaxies in order to strengthen the zero-point calibration. Ultimately we can reach the Virgo Cluster through a distance ladder with only three rungs: subdwarf parallaxes, Milky Way globular clusters, and then directly to Virgo (with HST).
dc.description14 pages, 6 eps figures. To appear in "The Extragalactic Distance Scale", eds. M. Livio, M. Donahue, and N. Panagia (Cambridge University Press)
dc.identifierhttps://arxiv.org/abs/astro-ph/9702008
dc.identifierhttp://arxiv.org/abs/astro-ph/9702008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11031
dc.subjectAstrophysics
dc.titlePost-AGB Stars as Standard Extragalactic Candles
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