期刊
ASTROPHYSICAL JOURNAL
卷 852, 期 2, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.3847/1538-4357/aa9e53
关键词
galaxies: active; galaxies: ISM; galaxies: nuclei; radiative transfer; radio lines: ISM
资金
- JSPS KAKENHI [16H03959, 17K14247]
- Grants-in-Aid for Scientific Research [16H03959, 15K05032, 17K14247] Funding Source: KAKEN
In this study, we investigate the line emissions from cold molecular gas based on our previous radiation-driven fountain model, which reliably explains the spectral energy distribution of the nearest type 2 Seyfert galaxy, the Circinus galaxy. Using a snapshot of the best-fit radiation-hydrodynamic model for the central r <= 16 pc, in which non-equilibrium X-ray-dominated region chemistry is solved, we conduct post-processed non-local thermodynamic equilibrium radiation transfer simulations for the CO lines. We obtain a spectral line energy distribution with a peak around J similar or equal to 6, and its distribution suggests that the lines are not thermalized. However, for a given line of sight, the optical depth distribution is highly non-uniform between tau(nu) << 1 and tau(nu) >> 1. The CO-to-H-2 conversion factor (XCO), which can be directly obtained from the results and is not a constant, depends strongly on the integrated intensity and differs from the fiducial value for local objects. XCO exhibits a large dispersion of more than one order of magnitude, reflecting the non-uniform internal structure of a torus. In addition, we found that the physical conditions differ between grid cells on a scale of a few parsecs along the observed lines of sight; therefore, a specific observed line ratio does not necessarily represent a single physical state of the interstellar medium.
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