Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aj....108..851r&link_type=abstract
The Astronomical Journal, vol. 108, no. 3, p. 851-861
Astronomy and Astrophysics
Astronomy
6
Cosmology, Hydrogen, Infrared Astronomy, Infrared Astronomy Satellite, Line Spectra, Mass, Near Infrared Radiation, Red Shift, Sampling, Sky Surveys (Astronomy), Spatial Distribution, Spectrum Analysis, Spiral Galaxies, Algorithms, Correlation, Data Reduction, Distance, Monte Carlo Method, Random Errors, Signal To Noise Ratios, Tables (Data), Variations, Velocity
Scientific paper
We have extracted a volume-limited sample of spiral galaxies within 4000 km/s from the Strauss et al. (1992) redshift survey of Infrared Astronomical Satellite (IRAS) galaxies. The purpose of the sample is to use distances obtained from the neutral hydrogen/near-infrared (I-band) Tully-Fisher relation to study deviations from uniform Hubble expansion. This will allow us to estimate the distribution of mass in the local universe and to place constraints on the value of the cosmological density parameter, omega 0. Here we report neutral hydrogen (H I) observations of 61 galaxies from this sample taken at the 64 m Parkes telescope, 48 of which resulted in measured linewidth parameters. Empirical estimates of random and systematic errors in H I line widths at low signal-to-noise ratio are described.
Mould Jeremy
Roth Joshua
Staveley--Smith Lister
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