A ghostly damped Ly α system revealed by metal absorption lines. (16th November 2016)

• Record Type: Journal Article
• Authors: Fathivavsari, H.; Petitjean, P.; Zou, S.; Noterdaeme, P.; Ledoux, C.; Krühler, T.; Srianand, R.
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 466:Number 1(2017:Mar.)
• Page Start: L58
• Page End: L62
• Publication Date: 2016-11-16
• Subjects: quasars: absorption lines -- quasars: emission lines -- quasars: individual: SDSS J113341.29−005740.0; Astronomy -- Research -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnrasl/slw233
• Languages: English
• ISSNs: 1745-3933

Abstract

Abstract: We report the discovery of the first 'ghostly' damped Ly α absorption system (DLA), which is identified by the presence of absorption from strong low-ion species at z abs = 1.704 65 along the line of sight to the quasar SDSS J113341.29−005740.0 with z em = 1.704 41. No Ly α absorption trough is seen associated with these absorptions because the DLA trough is filled with the leaked emission from the broad emission-line region of the quasar. By modelling the quasar spectrum and analysing the metal lines, we derive log N (H i )(cm −2 ) ∼21.0 ± 0.3. The DLA cloud is small (≤0.32 pc), thus not covering entirely the broad-line region and is located at ≥39 pc from the central active galactic nucleus (AGN). Although the DLA is slightly redshifted relative to the quasar, its metallicity ([S/H] = −0.41 ± 0.30) is intermediate between what is expected from infalling and outflowing gas. It could be possible that the DLA is part of some infalling material accreting on to the quasar host galaxy through filaments, and that its metallicity is raised by mixing with the enriched outflowing gas emanating from the central AGN. Current DLA surveys miss these 'ghostly' DLAs, and it would be important to quantify the statistics of this population by searching the Sloan Digital Sky Survey (SDSS) data base using metal absorption templates.