Multi-Sightline Observation of Narrow Absorption Lines in Lensed Quasar SDSS J1029+2623
arXiv:1605.04775 · doi:10.3847/0004-637X/825/1/25
Abstract
We exploit the widely-separated images of the lensed quasar SDSS J1029+2623 (=2.197, ) to observe its outflowing wind through two different sightlines. We present an analysis of three observations, including two with the Subaru telescope in 2010 February (Misawa et al. 2013) and 2014 April (Misawa et al. 2014), separated by 4 years, and one with the Very Large Telescope, separated from the second Subaru observation by 2 months. We detect 66 narrow absorption lines (NALs), of which 24 are classified as intrinsic NALs that are physically associated with the quasar based on partial coverage analysis. The velocities of intrinsic NALs appear to cluster around values of 59,000, 43,000, and 29,000 km/s, which is reminiscent of filamentary structures obtained by numerical simulations. There are no common intrinsic NALs at the same redshift along the two sightlines, implying that the transverse size of the NAL absorbers should be smaller than the sightline distance between two lensed images. In addition to the NALs with large ejection velocities of > 1,000 km/s, we also detect broader proximity absorption lines (PALs) at . The PALs are likely to arise in outflowing gas at a distance of r 620 pc from the central black hole with an electron density of 8.710 cm. These limits are based on the assumption that the variability of the lines is due to recombination. We discuss the implications of these results on the three-dimensional structure of the outflow.
23 pages, including 13 figures; accepted for publication in the Astrophysical Journal. A complete version with all tables and figures is available at http://www.shinshu-u.ac.jp/faculty/general/chair/astro/arXiv/sdss1029.pdf
References in corpus (14)
- Quasar Broad Absorption Line Variability on Multi-Year Time Scales
- A Census of Intrinsic Narrow Absorption Lines in the Spectra of Quasars at z=2-4
- Tombaugh 2: The First Open Cluster with a Significant Abundance Spread or Embedded in a Cold Stellar Stream?
- The Quasar-frame Velocity Distribution of Narrow CIV Absorbers
- The AGN Outflow in the HDFS Target QSO J2233-606 from a High-Resolution VLT/UVES Spectrum
- Line-driven radiative outflows in luminous quasars
- A Two-Year Time Delay for the Lensed Quasar SDSS J1029+2623
- The Third Image of the Large-Separation Lensed Quasar SDSS J1029+2623
- Monitoring the Variability of Intrinsic Absorption Lines in Quasar Spectra
- HST/COS observations of a new population of associated QSO absorbers
- Lens-Aided Multi-Angle Spectroscopy (LAMAS) Reveals Small-Scale Outflow Structure in Quasars
- Narrow absorption lines with two observations of Sloan Digital Sky Survey
- Resolving the Clumpy Structure of the Outflow Winds in the Gravitationally Lensed Quasar SDSS J1029+2623
- On the Covering Fraction Variability in an EUV Mini-BAL Outflow from PG 1206+459
Cited by in corpus (6)
- Narrow absorption lines complex I: one form of broad absorption line
- The correlated variations of C IV narrow absorption lines and quasar continuum
- COOL-LAMPS III: Discovery of a 25".9 Separation Quasar Lensed by a Merging Galaxy Cluster
- Narrow Absorption Lines Complex. II. Probing the Line-locking Signatures within the Trough-like Broad Absorption Line
- The X-Rays wind connection in PG 2112+059
- Spectroscopic Observations of the Outflowing Wind in the Lensed Quasar SDSS J1001+5027