Physics Reports vol.333, 334

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494 (1998) 118. N. Panagia, 1998 STScI preprint No. 1218. A. Walker, Post-Hipparcos Cosmic Candles, Kluwer Academic Publishers, the Netherlands, 1999, p. 125. L. Turner, R. P. Ostriker, Astron. J. 103 (1992) 1427. X. S. Turner, Astrophys. J. 493 (1997) 519. Y. N. L. Turner, Astrophys. J. 498 (1998) 1. A. , Astrophys. J. 419 (1993) 1. J. , Astrophys. J. 420 (1994) 455. M. Turner, in 1990 Nobel Symposium: The Birth and Early Evolution of Our Universe, Dark Matter in the Universe, 1991. P. R. Ellis, Nature 370 (1994) 609.

Conclusions: work in progress Where do we go from here? The results of recent years suggest younger ages than previously determined for globular clusters, and also give us more reliable estimates of the uncertainties in the presumed ages, just as David would have liked. Nevertheless, the current results, while barely marginally consistent with a #at matter-dominated Universe for the recent HST Key Project Hubble constant measurement, are still consistent with a vast range of cosmological models.

Lett. 413 (1993) 105. B. R. Fisher, Astron. Astrophys. 54 (1977) 661. M. Aaronson, G. Bothun, J. Mould, J. A. E. Cornell, Astrophys. J. 302 (1986) 536. J. B. Tully, Astrophys. J. 330 (1988) 579. R. P. P. Vogt, G. J. N. Da Costa, W. Freudling, Astron. J. 113 (1997) 22. M. E. Jackson, Astrophys. J. 204 (1976) 668. A. Dressler, D. Lynden-Bell, D. L. M. Faber, R. Terlevich, G. Wegner, Astrophys. J. 313 (1987) 37. G. Djorgovski, M. Davis, Astrophys. J. 313 (1987) 59. I. Jorgensen, M. Franx, P. Kjaergaard, Mon.

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