Preprint
Does the HCN/CO ratio trace the star-forming fraction of gas? I. A comparison with analytical models of star formation
Abstract
We use archival ALMA observations of the HCN and CO $J=1-0$ transitions, in
addition to the radio continuum at 93 GHz, to assess the relationship between
Authors
Bemis AR; Wilson CD
Publication date
January 16, 2023
DOI
10.48550/arxiv.2301.06478
Preprint server
arXiv