The MG II absorption system in the QSO PKS 2128-12 - A galaxy disc/halo with a radius of 65 KPC

Astronomy and Astrophysics – Astrophysics

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Absorption Spectra, Disk Galaxies, Intergalactic Media, Interstellar Gas, Metallicity, Quasars, Astronomical Spectroscopy, Cosmology, Galactic Structure, Magnesium, Red Shift

Scientific paper

An imaging survey of the field around QSO PKS 2128-12, a QSO with low redshift narrow Mg II absorption line systems, is performed to verify the assumption that sharp metal-rich absorption systems found in the spectra of QSO's arise in intervening materials. The absorber has a redshift, z = 0.4299, that is smaller than that of the QSO emission redshift. The closest galaxy to the QSO, lies 64 kpc north-east of it, and has a redshift equal to that of the absorber. It is gas-rich, and its V and red magnitudes are about those expected for a spiral galaxy. Since the absorbing gas is found to have a small velocity dispersion, fairly high abundances and column densities, and a moderate degree of ionization, it is more likely associated with material in the disc of this galaxy than with a large surrounding halo. This QSO-galaxy pair increases by a factor of four the projected distance from a galaxy center at which absorbing ionized gas has been detected, strongly favoring the assumption of intervening galaxies at least for moderately ionized absorbers.

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