PRUSSIC II -- ALMA imaging of dense-gas tracers in SDP.81: Evidence for low mechanical heating and a sub-solar metallicity in a z=3.04 dusty galaxy

TL;DR

This study uses ALMA observations of dense-gas tracers in a high-redshift galaxy to reveal low mechanical heating and sub-solar metallicity, impacting our understanding of galaxy evolution at z=3.04.

Contribution

First detection of HCO+(4-3) in a high-redshift galaxy and analysis indicating low mechanical heating and sub-solar metallicity in SDP.81.

Findings

HCO+(4-3) detected and resolved, HCN(4-3) and HNC(4-3) not detected

High HCO+/HCN ratio suggests low mechanical heating and low metallicity

Detection of CO(0-1) absorption and CO(1-0) emission from a companion galaxy

Abstract

We present deep ALMA Band 3 observations of the HCN, HCO+, and HNC (4-3) emission in SDP.81, a well-studied z = 3.042 strongly lensed galaxy. These lines trace the high-density gas, which remains almost entirely unexplored in z$\geq$1 galaxies. Additionally, these dense-gas tracers are potentially powerful diagnostics of the mechanical heating of the interstellar medium. While the HCN(4-3) and HNC(4-3) lines are not detected, the HCO+(4-3) emission is clearly detected and resolved. This is the third detection of this line in a high-redshift star-forming galaxy. We find an unusually high HCO+/HCN intensity ratio of $\geq$2.2. Based on the photodissociation region modelling, the most likely explanation for the elevated HCO+/HCN ratio is that SDP.81 has low mechanical heating - less than 10% of the total energy budget - and a sub-solar metallicity, Z=0.5 Z$_\odot$. While such conditions might not be representative of the general population of high-redshift dusty galaxies, lower-than-solar metallicity might have a significant impact on gas masses inferred from CO observations. In addition, we report the detection of CO(0-1) absorption from the foreground lensing galaxy and CO(1-0) emission from a massive companion to the lensing galaxy, approximately 50 kpc to the southeast.