The Correlation Between Galaxy HI Linewidths and K' Luminosities
Abstract
The relationship between galaxy luminosities and rotation rates is studied with total luminosities in the K' band. Extinction problems are essentially eliminated at this band centered at 2.1 micron. A template luminosity-linewidth relation is derived based on 65 galaxies drawn from two magnitude-limited cluster samples. The zero-point is determined using 4 galaxies with accurately known distances. The calibration is applied to give the distance to the Pisces Cluster (60 Mpc) at a redshift in the CMB frame of 4771 km/s. The resultant value of the Hubble Constant is 81 km/s/Mpc. The largest sources of uncertainty arises from the small number of zero-point calibrators at this time at K' and present application to only one cluster.
Cite
@article{arxiv.astro-ph/9911053,
title = {The Correlation Between Galaxy HI Linewidths and K' Luminosities},
author = {B. Rothberg and W. Saunders and R. B. Tully and P. L. Witchalls},
journal= {arXiv preprint arXiv:astro-ph/9911053},
year = {2009}
}
Comments
13 pages including 5 figures and 2 tables. Accepted for publication in Astrophysical Journal