A Quasar Shedding Its Dust Cocoon at Redshift 2
Journal Article
·
· The Astrophysical Journal
- Chinese Academy of Sciences (CAS), Kunming (China). Yunnan Observatories and Key Laboratory for the Structure and Evolution of Celestial Objects; Pennsylvania State Univ., University Park, PA (United States)
- Pennsylvania State Univ., University Park, PA (United States)
- Peking Univ., Beijing (China)
- Nanjing Univ. (China)
- Univ. of Nevada, Reno, NV (United States)
- Univ. of Arizona, Tucson, AZ (United States). Steward Observatory
- Univ. of Science and Technology of China, Hefei (China)
- Sun Yat-Sen Univ., Zhuhai (China)
- Chinese Academy of Sciences (CAS), Kunming (China). Yunnan Observatories and Key Laboratory for the Structure and Evolution of Celestial Objects
We present the first near-IR spectroscopy and joint analyses of multiwavelength observations for SDSS J082747.14+425241.1, a dust-reddened, weak broad emission-line quasar (WLQ) undergoing a remarkable broad-absorption line (BAL) transformation. The systemic redshift is more precisely measured to be z = 2.070 ± 0.001 using Hβ compared to z = 2.040 ± 0.003 using Mg ιι from the literature, signifying an extreme Mg ιι blueshift of 2140 ± 530 km s–1 relative to Hβ. Using the Hβ-based single-epoch scaling relation with a systematic uncertainty of 0.3 dex, its black hole (BH) mass and Eddington ratio are estimated to be MBH ~ 6.1 × 108M⊙ and λEdd ~ 0.71, indicative of being in a rapidly accreting phase. Our investigations confirm the WLQ nature and the LoBAL → HiBAL transformation, along with a factor of 2 increase in the Mg ιι+Fe ιι emission strength and a decrease of 0.1 in E(B – V) over two decades. The kinetic power of this LoBAL wind at R ~ 15 pc from its BH is estimated to be ~43% of the Eddington luminosity, sufficient for quasar feedback upon its host galaxy albeit with an order-of-magnitude uncertainty. This quasar provides a clear example of the long-sought scenario where LoBAL quasars are surrounded by dust cocoons, and wide-angle nuclear winds play a key role in the transition of red quasars evolving into the commonly seen blue quasars.
- Research Organization:
- US Department of Energy (USDOE), Washington, DC (United States). Office of Science, Sloan Digital Sky Survey (SDSS)
- Sponsoring Organization:
- CXC; China Manned Space Project; Chinese Academy of Sciences (CAS); National Key Research and Development Program of China; National Science Foundation (NSF); National Science Foundation of China (NSFC); USDOE Office of Science (SC)
- OSTI ID:
- 1983252
- Journal Information:
- The Astrophysical Journal, Journal Name: The Astrophysical Journal Journal Issue: 1 Vol. 930; ISSN 0004-637X
- Publisher:
- IOP PublishingCopyright Statement
- Country of Publication:
- United States
- Language:
- English
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