Gaseous Extent of Galaxies and the Origin of QSO Absorption Systems

Mathematics – Logic

Scientific paper

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Scientific paper

I present a study of the galaxies that give rise to Lyman-α (Lyα ) and triply ionized carbon (C IV) absorption lines observed in the spectra of background quasi-stellar objects. By comparing the redshifts of galaxies and Lyα absorption systems along common lines of sight, I confirmed the existence of an anti-correlation between Lyα absorption equivalent width and galaxy impact parameter. Further analysis showed that the extent of tenuous gas scales with galaxy B-band and K-band luminosities. I found that extended gaseous halos are a common and generic feature of galaxies over a wide range of luminosity and morphological type and Lyα absorption systems traced a significant and representative portion of the galaxy population. By comparing the redshifts of galaxies and C IV absorption systems along common lines of sight, I also found that extended gaseous halos of galaxies have been enriched by metals out to large galactocentric radii, ≈ 100\ h-1 kpc. The covering factor of ionized gas in galactic halos was estimated to nearly unity.

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