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HD 4343


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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:Phénix
Right ascension:00h45m20.26s
Declination:-48°50'10.0"
Apparent magnitude:7.614
Distance:160.514 parsecs
Proper motion RA:62.9
Proper motion Dec:17.1
B-T magnitude:7.95
V-T magnitude:7.642

Catalogs and designations:
Proper Names   (Edit)
HD 1989HD 4343
TYCHO-2 2000TYC 8034-1211-1
USNO-A2.0USNO-A2 0375-00235313
HIPHIP 3548

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