NASA/IPAC EXTRAGALACTIC DATABASE
Date and Time of the Query: 2019-01-24 T03:21:02 PST
Help | Comment | NED Home

For refcode 1997AJ....113...22G:
Retrieve 808 NED objects in this reference.
Please click here for ADS abstract

NED Abstract

Copyright by American Astronomical Society. Reproduced by permission
1997AJ....113...22G THE I BAND TULLY-FISHER RELATION FOR CLUSTER GALAXIES: DATA PRESENTATION RICCARDO GIOVANELLI, MARTHA P. HAYNES, TERRY HERTER, AND NICOLE P. VOGT Center for Radiophysics and Space Research and National Astronomy and Ionosphere Center, Cornell University, Ithaca, New York 14853 Electronic mail: riccardo@astrnsun.tn.cornell.edu, haynes@astrosun.tn.cornell.edu, herter@astrosun.tn.cornell.edu, nicole@lick.ucsc.edu GARY WEGNER Department of Physics and Astronomy, Dartmouth College, Hanover, New Hampshire 03755 Electronic mail: wegner@kayz.dartmouth.edu JOHN J. SALZER Department of Astronomy, Wesleyan University, Middletown, Connecticut 06459 Electronic mail: slaz@parcha.astro.wesleyan.edu LUIZ N. DA COSTA European Southern Observatory, Karl Schwarzschild Strasse 2, D-85748 Garching b. Munchen, Germany Electronic mail: ldaoosta@eso.org WOLFRAM FREUDLING Space Telescope-European Coordinating Facility, Karl Schwarzschild Strasse 2, D-85748 Garching b. Munchen, Germany Electronic mail: wfreudli@eso.org Received 1996 July 18; revised 1996 October 17 ABSTRACT 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 24 clusters or groups. J band photometry for the full sample was either obtained by us or compiled from published literature. Rotational velocities are derived either from 21 cm spectra or optical emission line long-slit spectra, and converted to a homogeneous scale. In addition to presenting the data, a discussion of the various sources of error on TF parameters is introduced, and the criteria for the assignment of membership to each cluster are given.
Retrieve 808 NED objects in this reference.
Please click here for ADS abstract

Back to NED Home