Using CO line ratios to trace the physical properties of molecular clouds

Peñaloza, Camilo H., Clark, Paul C. ORCID: https://orcid.org/0000-0002-4834-043X, Glover, Simon C. O., Shetty, Rahul and Klessen, Ralf S. 2017. Using CO line ratios to trace the physical properties of molecular clouds. Monthly Notices of the Royal Astronomical Society 465 (2) , pp. 2277-2285. 10.1093/mnras/stw2892

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Abstract

The carbon monoxide (CO) rotational transition lines are the most common tracers of molecular gas within giant molecular clouds (MCs). We study the ratio (R2–1/1–0) between CO’s first two emission lines and examine what information it provides about the physical properties of the cloud. To study R2–1/1–0, we perform smooth particle hydrodynamic simulations with timedependent chemistry (using GADGET-2), along with post-process radiative transfer calculations on an adaptive grid (using RADMC-3D) to create synthetic emission maps of a MC. R2–1/1–0 has a bimodal distribution that is a consequence of the excitation properties of each line, given that J = 1 reaches local thermal equilibrium while J = 2 is still sub-thermally excited in the considered clouds. The bimodality of R2–1/1–0 serves as a tracer of the physical properties of different regions of the cloud, and it helps constrain local temperatures, densities and opacities. Additionally, this bimodal structure shows an important portion of the CO emission comes from diffuse regions of the cloud, suggesting that the commonly used conversion factor of R2–1/1–0 ∼ 0.7 between both lines may need to be studied further

Item Type:	Article
Date Type:	Publication
Status:	Published
Schools:	Physics and Astronomy Advanced Research Computing @ Cardiff (ARCCA)
Publisher:	Oxford University Press
ISSN:	0035-8711
Date of First Compliant Deposit:	14 July 2017
Date of Acceptance:	7 November 2016
Last Modified:	05 May 2023 16:37
URI:	https://orca.cardiff.ac.uk/id/eprint/102453

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