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The Tully-Fisher Relation and H_not
R. Giovanelli, M. Haynes, L. da Costa +3
The use of the Tully-Fisher (TF) relation for the determination of the Hubble Constant relies on the availability of an adequate template TF relation and of reliable primary distan…
A Test of the Lauer--Postman Bulk Flow
Riccardo Giovanelli, Martha P. Haynes, Gary Wegner +3
We use Tully--Fisher distances for a sample of field late spiral galaxies to test the Lauer and Postman (1994; hereinafter LP) result suggestive of a bulk flow with respect to the…
Deviations from Hubble Flow in the Local Universe
Riccardo Giovanelli
Reviews observational situation in the measurement of peculiar velocities in the local universe. Emphasis is placed on such topics as: Do spirals and ellipticals yield the same pec…
The I-Band Tully-Fisher Relation for Cluster Galaxies: a Template Relation, its Scatter and Bias Corrections
R. Giovanelli, M. Haynes, T. Herter +5
Infrared I band photometry and velocity widths for galaxies in 24 clusters, with radial velocities between 1,000 and 10,000 \kms, are used to construct a template Tully--Fisher (TF…
The I-Band Tully-Fisher Relation for Cluster Galaxies: Data Presentation
R. Giovanelli, M. Haynes, T. Herter +5
Observational parameters which can be used for redshift-independent distance determination using the Tully-Fisher (TF) technique are given for 782 spiral galaxies in the fields of…
The I-Band Tully-Fisher Relation and the Hubble Constant
Riccardo Giovanelli
The application of the I band Tully--Fisher relation towards determining the Hubble constant is reviewed, with particular attention to the impact of scatter and bias corrections in…