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astro-ph1998
The Identification of LyαAbsorbers at Low Redshift
Suzanne M. Linder
Plots of equivalent width (or neutral hydrogen column density) versus impact parameter (between the galaxy and quasar line of sight) have been used to support a variety of conclusi…
astro-ph1998
Simulations of LyαAbsorption from Low Surface Brightness Galaxies
Suzanne M. Linder
Using simulations of the low redshift galaxy population based upon galaxy observations, it is shown (Linder 1998) that the majority of Ly absorbers at low redshift could arise i…