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

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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 stud...

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Bibliographic Details
Main Authors: Peñaloza, Camilo H. (Author) , Glover, Simon (Author) , Shetty, Rahul (Author) , Klessen, Ralf S. (Author)
Format: Article (Journal)
Language:English
Published: 12 November 2016
In: Monthly notices of the Royal Astronomical Society
Year: 2017, Volume: 465, Issue: 2, Pages: 2277-2285
ISSN:1365-2966
DOI:10.1093/mnras/stw2892
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stw2892
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Author Notes:Camilo H. Peñaloza, Paul C. Clark, Simon C.O. Glover, Rahul Shetty and Ralf S. Klessen
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Summary: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 time-dependent 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 Description:Gesehen am 26.10.2017
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stw2892

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