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• W4200370829 endingPage "773" @default.
• W4200370829 startingPage "753" @default.
• W4200370829 abstract "The properties of synthetic CO emission from 3D simulations of forming molecular clouds are studied within the SILCC-Zoom project. Since the time scales of cloud evolution and molecule formation are comparable, the simulations include a live chemical network. Two sets of simulations with an increasing spatial resolution (d$x=3.9$ pc to d$x=0.06$ pc) are used to investigate the convergence of the synthetic CO emission, which is computed by post-processing the simulation data with the RADMC-3D radiative transfer code. To determine the excitation conditions, it is necessary to include atomic hydrogen and helium alongside H$_2$, which increases the resulting CO emission by ~7-26 per cent. Combining the brightness temperature of $^{12}$CO and $^{13}$CO, we compare different methods to estimate the excitation temperature, the optical depth of the CO line and hence, the CO column density. An intensity-weighted average excitation temperature results in the most accurate estimate of the total CO mass. When the pixel-based excitation temperature is used to calculate the CO mass, it is over-/underestimated at low/high CO column densities where the assumption that $^{12}$CO is optically thick while $^{13}$CO is optically thin is not valid. Further, in order to obtain a converged total CO luminosity and hence <$X_{rm CO}$> factor, the 3D simulation must have d$xlesssim0.1$ pc. The <$X_{rm CO}$> evolves over time and differs for the two clouds; yet pronounced differences with numerical resolution are found. Since high column density regions with a visual extinction larger than 3~mag are not resolved for d$xgtrsim 1$~pc, in this case the H$_2$ mass and CO luminosity both differ significantly from the higher resolution results and the local $X_{rm CO}$ is subject to strong noise. Our calculations suggest that synthetic CO emission maps are only converged for simulations with d$xlesssim 0.1$ pc." @default.
• W4200370829 created "2021-12-31" @default.
• W4200370829 creator A5018273831 @default.
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• W4200370829 creator A5078285187 @default.
• W4200370829 creator A5087614869 @default.
• W4200370829 date "2021-11-23" @default.
• W4200370829 modified "2023-09-30" @default.
• W4200370829 title "Synthetic CO emission and the <i>X</i>CO factor of young molecular clouds: a convergence study" @default.
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• W4200370829 doi "https://doi.org/10.1093/mnras/stab3354" @default.
• W4200370829 hasPublicationYear "2021" @default.
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