# CIRCUMNUCLEAR MOLECULAR GAS IN MEGAMASER DISK GALAXIES NGC 4388 AND NGC 1194

## Author(s): Greene, Jenny E.; Seth, Anil; Lyubenova, Mariya; Walsh, Jonelle; van de Ven, Glenn; et al

To refer to this page use: http://arks.princeton.edu/ark:/88435/pr18q8r
DC FieldValueLanguage
dc.contributor.authorGreene, Jenny E.-
dc.contributor.authorSeth, Anil-
dc.contributor.authorLyubenova, Mariya-
dc.contributor.authorWalsh, Jonelle-
dc.contributor.authorvan de Ven, Glenn-
dc.contributor.authorLaesker, Ronald-
dc.date.accessioned2019-10-09T19:32:59Z-
dc.date.available2019-10-09T19:32:59Z-
dc.date.issued2014-06-20en_US
dc.identifier.citationGreene, Jenny E, Seth, Anil, Lyubenova, Mariya, Walsh, Jonelle, van de Ven, Glenn, Laesker, Ronald. (2014). CIRCUMNUCLEAR MOLECULAR GAS IN MEGAMASER DISK GALAXIES NGC 4388 AND NGC 1194. ASTROPHYSICAL JOURNAL, 788 (10.1088/0004-637X/788/2/145en_US
dc.identifier.issn0004-637X-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr18q8r-
dc.description.abstractWe explore the warm molecular and ionized gas in the centers of two megamaser disk galaxies using K-band spectroscopy. Our ultimate goal is to determine how gas is funneled onto the accretion disk, here traced by megamaser spots on sub-parsec scales. We present NIR IFU data with a resolution of similar to 50 pc for two galaxies: NGC 4388 with VLT/SINFONI and NGC 1194 with Keck/OSIRIS+AO. The high spatial resolution and rich spectral diagnostics allow us to study both the stellar and gas kinematics as well as gas excitation on scales only an order of magnitude larger than the maser disk. We find a drop in the stellar velocity dispersion in the inner similar to 100 pc of NGC 4388, a common signature of a dynamically cold central component seen in many active nuclei. We also see evidence for noncircular gas motions in the molecular hydrogen on similar scales, with the gas kinematics on 100 parsec scales aligned with the megamaser disk. In contrast, the high ionization lines and Br gamma trace outflow along the 100 parsec-scale jet. In NGC 1194, the continuum from the accreting black hole is very strong, making it difficult to measure robust two-dimensional kinematics, but the spatial distribution and line ratios of the molecular hydrogen and Br gamma have consistent properties between the two galaxies.en_US
dc.language.isoen_USen_US
dc.relation.ispartofASTROPHYSICAL JOURNALen_US
dc.rightsFinal published version. Article is made available in OAR by the publisher's permission or policy.en_US
dc.titleCIRCUMNUCLEAR MOLECULAR GAS IN MEGAMASER DISK GALAXIES NGC 4388 AND NGC 1194en_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.1088/0004-637X/788/2/145-
dc.date.eissued2014-06-03en_US
dc.identifier.eissn1538-4357-
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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