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Paper detail

High-Velocity Bipolar Molecular Emission from an AGN Torus

We have detected in ALMA observations CO J = 6 - 5 emission from the nucleus of the Seyfert galaxy NGC 1068. The low-velocity (up to +/- 70 km/s relative to systemic) CO emission resolves into a 12x7 pc structure, roughly aligned with the nuclear radio source. Higher-velocity emission (up to +/- 400 km/s) is consistent with a bipolar outflow in a direction nearly perpendicular (roughly 80 degrees) to the nuclear disk. The position-velocity diagram shows that in addition to the outflow, the velocity field may also contain rotation about the disk axis. These observations provide compelling evidence in support of the disk-wind scenario for the AGN obscuring torus.

preprint2016arXivOpen access
Jack F. GallimoreMoshe ElitzurRoberto MaiolinoAlessandro MarconiChristopher P. O'DeaDieter LutzStefi A. BaumRobert NikuttaC. M. V. ImpellizzeriRichard DaviesAmy E. KimballEleonora Sani
astro-ph.GA
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Jack F. GallimoreMoshe ElitzurRoberto MaiolinoAlessandro MarconiChristopher P. O'DeaDieter LutzStefi A. BaumRobert NikuttaC. M. V. ImpellizzeriRichard DaviesAmy E. KimballEleonora Sani

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