Velocity shift of Mg ii and Al iii broad absorption lines in quasar SDSS J134444.33+315007.6. (23rd September 2020)

• Record Type: Journal Article
• Authors: Lu, Wei-Jian; Lin, Ying-Ru
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 499:Number 1(2020)
• Page Start: L58
• Page End: L61
• Publication Date: 2020-09-23
• Subjects: galaxies: active -- quasars: absorption lines -- quasars: individual (SDSS J1344+3150); Astronomy -- Research -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnrasl/slaa158
• Languages: English
• ISSNs: 1745-3933

Abstract

ABSTRACT: We report, for the first time, a synchronized velocity shift of Mg ii and Al iii broad absorption lines (BALs) in quasar SDSS J134444.33+315007.6 (hereafter, J1344+3150). We found this quasar from a sample of 134 Mg ii BAL quasars with multi-epoch observations. This quasar contains three low-ionization BAL systems, the fastest of which at ${\sim} -17\, 000\, \rm km\, s^{-1}$ shows a kinematic shift of ${\sim} -1101$ and $\sim -1170\, \rm km\, s^{-1}$ in its Mg ii and Al iii ions, respectively, during a rest-frame time of about 3.21 yr. Meanwhile, this quasar also shows other various variation characteristics, including an obvious weakening in its continuum, a coordinated enhancement in multiple emission lines (Mg ii, C iii, and Al iii ), and a coordinated enhancement in three Al iii absorption troughs. These variation characteristics convincingly indicate that the BAL outflows of J1344+3150 are under the influence from the background radiation energy. Thus, we infer that the velocity shift displayed in system A in the quasar J1344+3150 may indicate an actual line-of-sight acceleration of an outflow due to the radiation pressure from the central source.