Circumnuclear Structures in Megamaser Host Galaxies

Patryk Pjanka, Jenny E. Greene, Anil C. Seth, James A. Braatz, Christian Henkel, Fred K.Y. Lo, Ronald Läsker

Research output: Contribution to journalArticle

5 Scopus citations

Abstract

Using the Hubble Space Telescope, we identify circumnuclear (100-500 pc scale) structures in nine new H2O megamaser host galaxies to understand the flow of matter from kpc-scale galactic structures down to the supermassive black holes (SMBHs) at galactic centers. We double the sample analyzed in a similar way by Greene et al. and consider the properties of the combined sample of 18 sources. We find that disk-like structure is virtually ubiquitous when we can resolve <200 pc scales, in support of the notion that non-axisymmetries on these scales are a necessary condition for SMBH fueling. We perform an analysis of the orientation of our identified nuclear regions and compare it with the orientation of megamaser disks and the kpc-scale disks of the hosts. We find marginal evidence that the disk-like nuclear structures show increasing misalignment from the kpc-scale host galaxy disk as the scale of the structure decreases. In turn, we find that the orientation of both the ∼100 pc scale nuclear structures and their host galaxy large-scale disks is consistent with random with respect to the orientation of their respective megamaser disks.

Original languageEnglish (US)
Article number165
JournalAstrophysical Journal
Volume844
Issue number2
DOIs
StatePublished - Aug 1 2017

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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    Pjanka, P., Greene, J. E., Seth, A. C., Braatz, J. A., Henkel, C., Lo, F. K. Y., & Läsker, R. (2017). Circumnuclear Structures in Megamaser Host Galaxies. Astrophysical Journal, 844(2), [165]. https://doi.org/10.3847/1538-4357/aa7c18