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arXiv · 1801.06332

The Megamaser Cosmology Project. X. High Resolution Maps and Mass Constraint for SMBHs

W. Zhao·J. A. Braatz·J. J. Condon·K. Y. Lo·M. J. Reid·C. Henkel·D. W. Pesce·J. E. Greene·F. Gao·C. Y. Kuo·C. M. V. Impellizzeri
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Abstract

We present high resolution (sub-mas) VLBI maps of nuclear H2O megamasers for seven galaxies. In UGC6093, the well-aligned systemic masers and high-velocity masers originate in an edge-on, flat disk and we determine the mass of the central SMBH to be M_SMBH = 2.58*10^7Msun(+-7%). For J1346+5228, the distribution of masers is consistent with a disk, but the faint high-velocity masers are only marginally detected, and we constrain the mass of the SMBH to be in the range 1.5-2.0*10^7Msun. The origin of the masers in Mrk1210 is less clear, as the systemic and high-velocity masers are misaligned and show a disorganized velocity structure. We present one possible model in which the masers originate in a tilted, warped disk, but we do not rule out the possibility of other explanations including outflow masers. In NGC6926, we detect a set of redshifted masers, clustered within a pc of each other, and a single blueshifted maser about 4.4pc away, an offset that would be unusually large for a maser disk system. Nevertheless, if it is a disk system, we estimate the enclosed mass to be M_SMBH<4.8*10^7 Msun . For NGC5793, we detect redshifted masers spaced about 1.4pc from a clustered set of blueshifted features. The orientation of the structure supports a disk scenario as suggested by Hagiwara et al.(2001). We estimate the enclosed mass to be M SMBH<1.3*10^7 Msun. For NGC2824 and J0350-0127, the masers may be associated with pc or sub-pc scale jets or outflows.

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W. Zhao, J. A. Braatz, J. J. Condon, K. Y. Lo, M. J. Reid, C. Henkel, D. W. Pesce, J. E. Greene, F. Gao, C. Y. Kuo, C. M. V. Impellizzeri. 2018-01-19. The Megamaser Cosmology Project. X. High Resolution Maps and Mass Constraint for SMBHs. https://doi.org/10.3847/1538-4357%2Faaa95c

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