2020/03/31 by Wei Zheng
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Emission spectrum #Galaxies: Formation, Evolution, Phenomena #Galaxy #Line-of-sight #OVV quasar #Physics #Quasar #Spectral line #Stellar, planetary, and galactic studies #astro-ph.CO #astro-ph.GA
paper · pdf · doi:10.3847/1538-4357/ab7b6f
published as The Astrophysical Journal, 892, 139 (2020) · 22 pages, 10 figures, 3 tables
openalex created_date 2020/03/06 · openalex publication_date 2020/04/01 · arxiv created 2020/04/07 · arxiv updated 2020/04/08 · openalex updated_date 2026/08/05
Abstract Insight into quasar ages may be obtained from the proximity effect, but so far only in a limited number of bright quasars. Based on ∼2600 Sloan Digital Sky Survey quasar spectra at 2.5 ≤ z ≤ 3.5, a search for spectral voids between Ly α forest lines finds proximity zones over a wide range of radial distances. The majority of zone sizes are less than 5 Mpc, with their numbers decreasing exponentially toward larger distances. After a normalization by luminosities, the zone sizes are distributed with an e-folding scale of 0.64 as compared with the anticipated values. A group of quasars are selected for their large proximity zones of ≳10 Mpc. Their composite spectrum displays strong narrow cores and large equivalent widths in Ly α and other major UV emission lines. If the proximity zones along lines of sight are indicative of quasar ages, these features may be the signatures of old quasars. Another group of quasars are selected as they show no proximity zone and exhibit intrinsic absorption lines at z ab > z em . They are likely young quasars and exhibit weaker narrow emission-line components. The significant difference of spectral features between the two groups may reflect an evolution pattern over quasars’ lifetimes.