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Cluster population incompleteness bias and the value of H(0) from the Tully-Fisher B0(T) relation
Data on the Virgo cluster and ten more distant clusters are the basis ofan evaluation of the influence of the cluster population incompletenessbias on the B-band Tully-Fisher relation. The data are well fitted by atheoretical curve that is obtained for a Hubble constant value of 72 +or - 5 km/sec per Mpc in the de Vaucouleurs local scale, confirming theconstant's previous determination in light of a study of the Malmquistbias for field galaxies. The true value for the Hubble constant isconcluded to lie within the 50-75 range, depending on the primarycalibration.
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Observation and Astrometry data
| Constellation: | Cetus |
| Right ascension: | 00h45m20.26s |
| Declination: | -05°00'32.7" |
| Apparent magnitude: | 8.719 |
| Distance: | 310.559 parsecs |
| Proper motion RA: | 11.5 |
| Proper motion Dec: | 10.3 |
| B-T magnitude: | 10.078 |
| V-T magnitude: | 8.832 |
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