Molecular properties of (U)LIRGs: CO, HCN, HNC and HCO+

@article{Loenen2007MolecularPO,
  title={Molecular properties of (U)LIRGs: CO, HCN, HNC and HCO+},
  author={Aede Folkert Loenen and Willem A. Baan and Marco Spaans},
  journal={Proceedings of the International Astronomical Union},
  year={2007},
  volume={3},
  pages={462 - 466}
}
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… Expand
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