paper

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

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