Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21460315t&link_type=abstract
American Astronomical Society, AAS Meeting #214, #603.15
Astronomy and Astrophysics
Astronomy
Scientific paper
The first large sample of absorption lines in the spectra of pairs of QSOs that are close in the sky contains some surprises. The absorbers in the paired QSOs have very similar redshifts, within 200 km/s, as if the absorption is from slow moving blue and not red galaxies. The absorption is not from winds flowing out of galaxies at high velocities, suggesting that the metals entered the intergalactic medium at earlier times.
We see no change in the absorption from neutral hydrogen in front of QSOs, and an increase in absorption to 6 Mpc behind QSOs. Either the QSO UV is emitted from the side facing us only, or these low luminosity QSOs emit for under 1 Myr at the intensity we seen. Supported by the NSF.
Chapman Angela
Crotts Arlin
Gleed Mark
Jena Tridivesh
Kirkman David
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