Intensity ratios for XDR/PDR identification

C. -E. Green,M. R. Cunningham,J. A. Green,J. R. Dawson,P. A. Jones,A. R. Lopez-Sanchez,L. Verdes-Montenegro,C. Henkel,W. A. Baan,S. Martin

IAU Symposium Proceedings Series（2015）

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摘要

The intensity ratios of HCO+/HCN and HNC/HCN (1-0) reveal the relative influence of star formation and active galactic nuclei (AGN) or black holes on the circum- nuclear gas of a galaxy, allowing the identification of X-ray dominated regions (XDRs) and Photon-dominated regions (PDRs). It is not always clear in the literature how this intensity ratio calculation has been, or should be performed. This paper discusses ratio calculation methods for interferometric data.

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关键词

astrochemistry,galaxies: active,galaxies: ISM,ISM: molecules,stars: formation

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