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5.13. High-density-and-temperature circumnuclear molecular torus in M51

  • S. Matsushita (a1), K. Kohno (a1), B. Vila-Vilaro (a1), R. Kawabe (a1) and T. Tosaki (a2)...

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It is very important to know the physical conditions of circumnuclear molecular gas in order to understand the nature of Active Galactic Nuclei (AGN), since the circumnuclear molecular gas in active galaxies might be directly affected by or is affecting the activity of nucleus. To investigate the physical conditions of the molecular clouds in detail, multi-line observations with millimeter arrays are essential.

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References

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Kohno, K., Kawabe, R., Tosaki, T. & Okumura, S. K. 1996, Ap.J., 461, L29.
Tacconi, L. J., Genzel, R., Blietz, M., Cameron, M., Harris, A. I., & Madden, S. 1994, Ap.J., 426, L77.
Wild, W., Harris, A.I., Eckart, A., Genzel, R., Graf, U.U., Jackson, J.M., Russell, A.P.G., & Stutzki, J. 1992, A&A, 265, 447.

5.13. High-density-and-temperature circumnuclear molecular torus in M51

  • S. Matsushita (a1), K. Kohno (a1), B. Vila-Vilaro (a1), R. Kawabe (a1) and T. Tosaki (a2)...

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