Weak 13CO in the Cloverleaf Quasar: evidence for a young, early generation starburst

TL;DR

This study presents the first detection of 13CO in a high-redshift quasar, suggesting a young, early starburst with a deficiency of secondary nuclei like 13CO, indicating rapid initial metal enrichment.

Contribution

It provides the first observational evidence of 13CO at high redshift and analyzes its implications for early galaxy chemical evolution.

Findings

13CO detected at high redshift in the Cloverleaf Quasar

High 12CO/13CO luminosity ratio suggests a deficiency of 13CO

LVG models indicate abundance ratios exceeding 100

Abstract

Observations of 12CO at high redshift indicate rapid metal enrichment in the nuclear regions of at least some galaxies in the early universe. However, the enrichment may be limited to nuclei that are synthesized by short-lived massive stars, excluding classical secondary nuclei like 13CO. Testing this idea, we tentatively detect the 13CO J=3-2 line at a level of 0.3 Jy km/s toward the Cloverleaf Quasar at redshift 2.5. This is the first observational evidence for 13CO at high redshift. The 12CO/13CO J=3-2 luminosity ratio is with at least 40 much higher than ratios observed in molecular clouds of the Milky Way and in the ultraluminous galaxy Arp 220, but may be similar to that observed toward NGC 6240. Large Velocity Gradient (LVG) models simulating seven 12CO transitions and the 13CO line yield 12CO/13CO abundance ratios in excess of 100 for the Cloverleaf. It is possible that the measured ratio is affected by a strong submillimeter radiation field, which reduces the contrast between the 13CO line and the background. It is more likely, however, that the ratio is caused by a real deficiency of 13CO. A potential conflict with optical data, indicating high abundances also for secondary nuclei in quasars of high redshift, may be settled if the bulk of the CO emission is originating sufficiently far from the active galactic nucleus.