ALMA Sub-parsec Resolution Dense Molecular Line Observations of the NGC 1068 Nucleus
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| Autores principales: | , , , , , |
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| Formato: | Preprint |
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2025
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| _version_ | 1866908635212283904 |
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| author | Imanishi, Masatoshi Vollmer, Bernd Hagiwara, Yoshiaki Nakanishi, Kouichiro Izumi, Takuma Kawakatu, Nozomu |
| author_facet | Imanishi, Masatoshi Vollmer, Bernd Hagiwara, Yoshiaki Nakanishi, Kouichiro Izumi, Takuma Kawakatu, Nozomu |
| contents | We present the results of our ALMA observations of the dense molecular HCN J=4-3 and HCO$^{+}$ J=4-3 lines at $\lesssim$1 pc ($\lesssim$14 mas) resolution in the nuclear region of the nearby ($\sim$14 Mpc) well-studied AGN NGC 1068. Both emission lines are clearly detected around the AGN along an almost east-west direction, which we ascribe to the dusty molecular torus. The HCN J=4-3 emission is brighter than the HCO$^{+}$ J=4-3 emission in the compact ($\lesssim$3-5 pc) torus region. Apparent counter-rotation between the inner ($\lesssim$2 pc) and outer ($\gtrsim$2 pc) parts of the western torus, previously seen in $\sim$1.5 pc-resolution HCN J=3-2 and HCO$^{+}$ J=3-2 data, is also confirmed in our new $\lesssim$1 pc-resolution HCN J=4-3 and HCO$^{+}$ J=4-3 data. We apply a physically counter-rotating torus model, in which a compact dense gas clump collided with the western side of the existing rotating torus from the opposite direction, and we find that this model largely reproduces the observed properties of the combined new $\lesssim$1 pc-resolution HCN J=4-3 and HCO$^{+}$ J=4-3 data, and the previously obtained $\lesssim$1.5 pc-resolution HCN J=3-2 and HCO$^{+}$ J=3-2 data. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2511_04772 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | ALMA Sub-parsec Resolution Dense Molecular Line Observations of the NGC 1068 Nucleus Imanishi, Masatoshi Vollmer, Bernd Hagiwara, Yoshiaki Nakanishi, Kouichiro Izumi, Takuma Kawakatu, Nozomu Astrophysics of Galaxies We present the results of our ALMA observations of the dense molecular HCN J=4-3 and HCO$^{+}$ J=4-3 lines at $\lesssim$1 pc ($\lesssim$14 mas) resolution in the nuclear region of the nearby ($\sim$14 Mpc) well-studied AGN NGC 1068. Both emission lines are clearly detected around the AGN along an almost east-west direction, which we ascribe to the dusty molecular torus. The HCN J=4-3 emission is brighter than the HCO$^{+}$ J=4-3 emission in the compact ($\lesssim$3-5 pc) torus region. Apparent counter-rotation between the inner ($\lesssim$2 pc) and outer ($\gtrsim$2 pc) parts of the western torus, previously seen in $\sim$1.5 pc-resolution HCN J=3-2 and HCO$^{+}$ J=3-2 data, is also confirmed in our new $\lesssim$1 pc-resolution HCN J=4-3 and HCO$^{+}$ J=4-3 data. We apply a physically counter-rotating torus model, in which a compact dense gas clump collided with the western side of the existing rotating torus from the opposite direction, and we find that this model largely reproduces the observed properties of the combined new $\lesssim$1 pc-resolution HCN J=4-3 and HCO$^{+}$ J=4-3 data, and the previously obtained $\lesssim$1.5 pc-resolution HCN J=3-2 and HCO$^{+}$ J=3-2 data. |
| title | ALMA Sub-parsec Resolution Dense Molecular Line Observations of the NGC 1068 Nucleus |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2511.04772 |