Slicing the cool circumgalactic medium along the major axis of a star-forming galaxy at z = 0.7. Issue 3 (14th November 2019)

• Record Type: Journal Article
• Authors: Lopez, S; Tejos, N; Barrientos, L F; Ledoux, C; Sharon, K; Katsianis, A; Florian, M K; Rivera-Thorsen, E; Bayliss, M B; Dahle, H; Fernandez-Figueroa, A; Gladders, M D; Gronke, M; Hamel, M; Pessa, I; Rigby, J R
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 491:Issue 3(2020)
• Page Start: 4442
• Page End: 4461
• Publication Date: 2019-11-14
• Subjects: galaxies: clusters: individual: PSZ1 G311.65–18.48 -- galaxies: evolution -- galaxies: formation -- intergalactic medium; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stz3183
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: We present spatially resolved Echelle spectroscopy of an intervening Mg ii –Fe ii –Mg i absorption-line system detected at z abs = 0.73379 towards the giant gravitational arc PSZ1 G311.65–18.48. The absorbing gas is associated with an inclined disc-like star-forming galaxy, whose major axis is aligned with the two arc-segments reported here. We probe in absorption the galaxy's extended disc continuously, at ≈3 kpc sampling, from its inner region out to 15× the optical radius. We detect strong ($W_0^{2796}\gt 0.3$ Å) coherent absorption along 13 independent positions at impact parameters D = 0–29 kpc on one side of the galaxy, and no absorption at D = 28–57 kpc on the opposite side (all de-lensed distances at z abs ). We show that (1) the gas distribution is anisotropic; (2) $W_0^{2796}$, $W_0^{2600}$, $W_0^{2852}$, and the ratio $W_0^{2600}\!/W_0^{2796}$, all anticorrelate with D ; (3) the $W_0^{2796}$ – D relation is not cuspy and exhibits significantly less scatter than the quasar-absorber statistics; (4) the absorbing gas is co-rotating with the galaxy out to D ≲ 20 kpc, resembling a 'flat' rotation curve, but at D ≳ 20 kpc velocities decline below the expectations from a 3D disc-model extrapolated from the nebular [O ii ] emission. These signatures constitute unambiguous evidence for rotating extra-planar diffuse gas, possibly also undergoing enriched accretion at its edge. Arguably, we are witnessing some of the long-sought processes of the baryon cycle in a single distant galaxy expected to be representative of such phenomena.