Significant H I and Metal Differences around the z = 0.83 Lens Galaxy Towards the Doubly Lensed Quasar SBS 0909+532
arXiv:2102.13523 · doi:10.3847/1538-3881/abd2b0
Abstract
We report a large difference in neutral hydrogen (H I) and metal column densities between the two sight lines probing opposite sides of the lensing galaxy at = 0.83 toward the doubly lensed quasar SBS 0909+532. Using archival HST-STIS and Keck HIRES spectra of the lensed quasar images, we measure log = 18.77 0.12 cm toward the brighter image () at an impact parameter of = 3.15 kpc and log = 20.38 0.20 cm toward the fainter image () at an impact parameter of = 5.74 kpc. This difference by a factor of 41 is the highest difference between sight lines for a lens galaxy in which H I has been measured, suggesting patchiness and/or anisotropy on these scales. We estimate an average Fe abundance gradient between the sight lines to be +0.35 dex kpc. The / ratios for the individual components detected in the Keck HIRES spectra have supersolar values for all components in sight line and for 11 out of 18 components in sight line , suggesting that Type Ia supernovae may have contributed to the chemical enrichment of the galaxy's environment. Additionally, these observations provide complementary information to detections of cold gas in early-type galaxies and the tension between these and some models of cloud survival.
20 pages, 6 tables, 11 figures
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