Lyman Alpha Absorption and Tidal Debris
arXiv:astro-ph/9311065 · doi:10.1086/174176
Abstract
It is suggested that a significant fraction of the low column-density absorption features seen in the spectra of quasars are produced in pressure-confined tidal debris, that was built up in small groups and clusters of galaxies over a Hubble time. We show that the space-density and cross-section of tidal tails in groups of galaxies are large enough that they could constitute a major source of the low redshift Ly absorption features that are associated with galaxies. The space-density of groups within 10 Mpc of our galaxy is found to be 2.4 Mpc, which is close to the Mpc space-density calculated for Ly absorbers, assuming they have a 1 Mpc radius. Other observational constraints on the properties of Ly absorber such as their velocity dispersion, correlation properties, dimensions and abundances, are shown to be consistent with this hypothesis.
6 pages, uuencodes compressed postscript, Accepted for publication in ApJ
Cited by in corpus (31)
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