arXiv · 0709.3423
Molecular properties of (U)LIRGs: CO, HCN, HNC and HCO+
Abstract
The observed molecular properties of a sample of FIR-luminous and OH megamaser (OH-MM) galaxies have been investigated. The ratio of high and low-density tracer lines is found to be determined by the progression of the star formation in the system. The HCO+/HCN and HCO+/HNC line ratios are good proxies for the density of the gas, and PDR and XDR sources can be distinguished using the HNC/HCN line ratio. The properties of the OH-MM sources in the sample can be explained by PDR chemistry in gas with densities higher than 10^5.5 cm^-3, confirming the classical OH-MM model of IR pumped amplification with (variable) low gains.
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A. F. Loenen, W. A. Baan, M. Spaans. 2007-09-21. Molecular properties of (U)LIRGs: CO, HCN, HNC and HCO+. https://doi.org/10.1017/s1743921307013609
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