VLA detects CO(1-0) emission in the z=3.65 quasar SDSS J160705+533558
arXiv:2202.07368 · doi:10.1051/0004-6361/202142682
Abstract
We present CO(1--0) observations of the high-redshift quasar SDSS J160705+533558 () using the Karl G. Jansky Very Large Array (VLA). We detect CO emission associated with the quasar and at projected distance from it, separated by in velocity. The total molecular gas mass of this system is . By comparing our CO detections with previous submillimetre (submm) observations of the source, an offset between the different emission components is revealed: the peak of the submm emission is offset from the quasar and from the CO companion detected in our VLA data. To explain our findings, we propose a scenario similar to that for the Antennae galaxies: SDSS J160705+533558 might be a merger system in which the quasar and the CO companion are the merging galaxies, whose interaction resulted in the formation of a dusty, star-forming overlap region between the galaxies that is dominant at the submm wavelengths.
5 pages, 3 figures, accepted for publication in Astronomy & Astrophysics
References in corpus (11)
- A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: I. Galaxy Mergers & Quasar Activity
- Rapidly star-forming galaxies adjacent to quasars at redshifts exceeding 6
- Host galaxies of luminous z0.6 quasars: Major mergers are not prevalent at the highest AGN luminosities
- ALMA Observations Show Major Mergers Among the Host Galaxies of Fast-growing, High-redshift Supermassive Black Holes
- The Discovery of Gas-Rich, Dusty Starbursts in Luminous Reddened Quasars at with ALMA
- ALMA observations of cold molecular gas in AGN hosts at z~1.5 - Evidence of AGN feedback?
- The redshift evolution of major merger triggering of luminous AGN: a slight enhancement at z2
- AGN feedback on molecular gas reservoirs in quasars at 2.4
- SMM J04135+10277: A distant QSO-starburst system caught by ALMA
- Towards an accurate model for the Antennae Galaxies
- ALMA detects molecular gas in the halo of the powerful radio galaxy TXS 0828+193