INTERIM REPORT ON THE HST KEY PROJECT TO MEASURE $H_0$

  • MOULD JEREMY (Mount Stromlo and Siding Springs Observatories Institute of Advanced Studies, Australian National University)
  • Published : 1996.12.01

Abstract

With an interim calibration based upon half the Key Project's galaxies, the Tully-Fisher relation, the (Dn, $\sigma$) relation and type II supernovae yield $H_0$= 73$\pm$10 km/sec/Mpc.

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