No CrossRef data available.
Published online by Cambridge University Press: 25 May 2016
Using B, V, R, I photometric parallaxes for components of wide binaries, new bolometric corrections by Bergeron et al. (1995) and cooling curves by Wood (1995), we have determined the white dwarf luminosity function (WDLF; Oswalt et al. 1996). A minimum age of 9.5+1.1−0.8 Gyr is implied for the Galactic disk; arbitrarily old models are consistent at the +2σ level. Smith (1997) confirms these results using a much larger sample and similar methodology. Using these same new models, Wood & Oswalt (1997) show that the WDLF of Liebert et al. (1988) yields an age of 7.5+0.5−0.5 Gyr, more than 20% younger than their original estimate.