Nature, Vol.377, No.6544, 27-31, 1995
Determination of the Hubble Constant from Observations of Cepheid Variables in the Galaxy M96
New Nubble Space Telescope observations of Cepheid variable stars in the nearby galaxy M96 give a distance to the host galaxy group, Leo I, of 11.6 +/- 0.8 Mpc. This value, used in conjunction with several reliable secondary indicators of relative distance, constrains the distances to more remote galaxy clusters, and yields a value of the Hubble constant (H-0 = 69 +/- 8 km s(-1) Mpc(-1)) that is independent of the velocity of the Leo I group itself.
Keywords:EXTRAGALACTIC DISTANCE SCALE;VIRGO CLUSTER;PLANETARY-NEBULAE;STANDARD CANDLES;ELLIPTICAL GALAXIES;PHOTOMETRY;UNIVERSE;AGE;SPECTROSCOPY;CATALOG