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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 Relative Distance between the Clusters of Galaxies A2634 and Coma
Marco Scodeggio, Riccardo Giovanelli, Martha P. Haynes
The Tully-Fisher and Fundamental Plane relations are used to obtain two independent estimates of the relative distance between the clusters A2634 and Coma. Previously published stu…
Two-Stream Instability of Counter-Rotating Galaxies
R. V. E. Lovelace, K. P. Jore, M. P. Haynes
The present study of the two-stream instability in stellar disks with counter-rotating components of stars and/or gas is stimulated by recently discovered counter-rotating spiral a…