Low-redshift Lyman-alpha absorption lines and the dark matter halos of disk galaxies

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Abstract
Ultraviolet observations of the lowredshift quasar 3C 273 using the Hubble Space Telescope have revealed many more Lyman-α absorption lines than would be expected from extrapolation of the absorption systems seen toward QSOs at z~2. Here I show that these absorption lines can plausibly be produced by gas at large radii in the disks of spiral and irregular galaxies; the gas is confined by the dark matter halos and ionized and heated by the extragalactic radiation field. This scenario does not require the extragalactic ionizing radiation field to decline as rapidly with decreasing z as the QSO emissivity. Observations of Lyα absorption through the halos of known galaxies at low redshift will constrain both the extragalactic background and the properties of galactic halos.

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