ALMA observations of a metal-rich damped Ly alpha absorber at z=2.5832: evidence for strong galactic winds in a galaxy group

作者：Fynbo J P U^*; Heintz K E^*; Neeleman M^*; Christensen L; Dessauges Zavadsky M; Kanekar N; Moller P; Prochaska J X; Rhodin N H P; Zwaan M

来源：Monthly Notices of the Royal Astronomical Society, 2018, 479(2): 2126-2132.

DOI：10.1093/mnras/sty1520

• galaxies: ISM
• ISM: molecules
• quasar: absorption lines
• quasars: individual (Q 0918+1636)
• submillimetre: ISM

We report on the results of a search for CO(3-2) emission from the galaxy counterpart of a high-metallicity Damped Ly alpha Absorber (DLA) at z= 2.5832 towards the quasar Q0918+1636. We do not detect CO emission from the previously identified DLA galaxy counterpart. The limit we infer on M-gas/M-* is in the low end of the range found for DLA galaxies, but is still consistent with what is found for other star-forming galaxies at similar redshifts. Instead we detect CO(3-2) emission from another intensely star-forming galaxy at an impact parameter of 117 kpc from the line of sight to the quasar and 131 km s(-1) redshifted relative to the velocity centroid of the DLA in the quasar spectrum. In the velocity profile of the low-and high-ionization absorption lines of the DLA there is an absorption component consistent with the redshift of this CO-emitting galaxy. It is plausible that this component is physically associated with a strong outflow in the plane of the sky from the CO-emitting galaxy. If true, this would be further evidence, in addition to what is already known from studies of Lyman-break galaxies, that galactic outflows can be traced beyond 100 kpc from star-forming galaxies. The case of this z = 2.583 structure is an illustration of this in a group environment.

• 出版日期2018-9