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For refcode 1988A&A...196...17B:
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Copyright by European Southern Observatory (ESO). Reproduced by permission
1988A&A...196...17B The value of H_0_ from the infrared Tully-Fisher relation L. Bottinelli, L. Gouguenheim, and P. Teerikorpi Observatoire de Paris, Section de Meudon, Departement de Radioastronomie, F-92195 Meudon Cedex, France Universite de Paris-Sud, Centre d'Orsay, F-91405 Orsay Cedex, France Turku University Observatory, Tuorla, SF-21500 Piikkio, Finland Received September 24, accepted November 17, 1987 Summary. Infrared H_0.5_ magnitudes and the Tully-Fisher method are used to study the value of the Hubble constant from field galaxies and clusters of galaxies. As in our previous studies using B^O^_T_-magnitudes, special attention is paid to the Malmquist and cluster population incompleteness biases. The slope of the direct TF relationship in the H-band is shown to be probably in the range 11.5-12.0. Both the field galaxies and the cluster galaxies provide values of H_0_ consistent with our previous determinations using the B-band: H_0_ lies in the range 70-75 km s^-1^ Mpc^-1^, when using de Vaucouleurs primary calibration. Key words: clusters of galaxies - distance - cosmology
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