Statistics – Computation
Scientific paper
Mar 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...326l...1b&link_type=abstract
Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 326, March 1, 1988, p. L1-L4. Research supported by
Statistics
Computation
32
Density Distribution, Galactic Evolution, Red Shift, Space Density, Computational Astrophysics, Spatial Distribution, Spiral Galaxies, Stellar Evolution
Scientific paper
The authors examine the effect of evolution on determinations of the density parameter from the distribution of galaxies in flux-redshift space. Their model separates galaxies into two classes, ellipticals and spirals, with different star formation histories, and includes a crude estimate of luminosity evolution due to accretion of satellite galaxies. It is found that the recent determination of the density parameter Ω0 by Loh and Spillar is uncertain by at least ΔΩ = ±1.
Bahcall Safi R.
Tremaine Scott
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