On the density regime probed by HCN emission

Jones, Gerwyn H., Clark, Paul C. ORCID: https://orcid.org/0000-0002-4834-043X, Glover, Simon C. O. and Hacar, Alvaro 2023. On the density regime probed by HCN emission. Monthly Notices of the Royal Astronomical Society 520 (1) , pp. 1005-1021. 10.1093/mnras/stad202

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Abstract

HCN J = 1 –0 emission is commonly used as a dense gas tracer, thought to mainly arise from gas with densities ∼104–105 cm−3. This has made it a popular tracer in star formation studies. However, there is increasing evidence from observational surveys of ‘resolved’ molecular clouds that HCN can trace more diffuse gas. We investigate the relationship between gas density and HCN emission through post-processing of high-resolution magnetohydrodynamical simulations of cloud–cloud collisions. We find that HCN emission traces gas with a mean volumetric density of ∼3 × 103 cm−3 and a median visual extinction of ∼5 mag.  We therefore predict a characteristic density that is an order of magnitude less than the ‘standard’ characteristic density of n ∼3 × 104 cm−3. Indeed, we find in some cases that there is clear HCN emission from the cloud even though there is no gas denser than this standard critical density. We derive independent luminosity-to-mass conversion factors for the amount of gas at AV > 8 or at densities n > 2.85 × 103 cm−3 or n > 3 × 104 cm−3, finding values of αHCN = 6.79, 8.62, and ⁠, 27.98 M (K km s−1 pc2 ),respectively.

Item Type:	Article
Date Type:	Publication
Status:	Published
Schools:	Schools > Physics and Astronomy
Publisher:	Oxford University Press
ISSN:	0035-8711
Date of First Compliant Deposit:	8 September 2025
Date of Acceptance:	16 January 2023
Last Modified:	08 Sep 2025 08:50
URI:	https://orca.cardiff.ac.uk/id/eprint/180961

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