Revealing the Gas Recycling in the Circumgalactic Medium (CGM) Utilizing a Luminous Ly$\alpha$ Nebula Around a Type-II Quasar at z=2.6 with the Keck Cosmic Web Imager (KCWI)
Shiwu Zhang, Zheng Cai, Dandan Xu, Andrea Afruni, Yunjing Wu, Wuji, Wang, Fabrizio Arrigoni Battaia, Mingyu Li, Sen Wang, Xianzhi Bi

TL;DR
This study uses KCWI observations of a Lyα nebula around a z=2.6 quasar to investigate gas recycling in the CGM, revealing diffuse emission, absorption features, and high metallicity, suggesting recycling over outflows.
Contribution
It provides new spectroscopic evidence of gas recycling in the CGM around a high-redshift quasar using integral field observations.
Findings
Diffuse Lyα, HeII, and CIV emission detected up to 122 kpc.
High metallicity (≥ Z⊙) of the cool CGM gas.
Gas recycling is a more plausible explanation than outflows.
Abstract
How galaxies acquire material from the circumgalactic medium (CGM) is a key question in galaxy evolution. Recent observations and simulations show that gas recycling could be an important avenue for star formation. This paper presents Keck Cosmic Web Imager (KCWI) integral field unit spectroscopic observations on a type-II quasar, Q1517+0055 at z = 2.65, a pilot study of our Ly nebulae sample at . We revealed diffuse emission of the Ly 1216, HeII 1640, and CIV 1549 on the projected physical scale of 122 kpc, 45 kpc, and 79 kpc, respectively. The total Ly luminosity is L = erg s. The line ratio diagnostics shows that HeII/Ly 0.08 and CIV/Ly 0.28, consistent with the photoionization including recombination and photon pumping. We also identify the associated HI and…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
