Abstract
HCN and CO in M51, HCN traces nucleus, HCN is brighter than COthe density and the temperature of the circumnuclear molecular gasare as high as 105 cm-3 and greater than 100 Kspectral lines, AGN torus, ALMA
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CITATION STYLE
APA
Matsushita, S., Kohno, K., Vila‐Vilaro, B., Tosaki, T., & Kawabe, R. (1998). High‐Density and High‐Temperature Circumnuclear Molecular Disk in M51. The Astrophysical Journal, 495(1), 267–275. https://doi.org/10.1086/305261
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