Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...155l...8b&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 155, no. 1, Jan. 1986, p. L8-L11.
Astronomy and Astrophysics
Astrophysics
78
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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