NIR imaging spectroscopy of the inner few arcseconds of NGC 4151 with OSIRIS at Keck
arXiv:1306.5627 · doi:10.1051/0004-6361/201219998
Abstract
We present H- and K-band data from the inner arcsecond of the Seyfert 1.5 galaxy NGC 4151 obtained with the adaptive optics assisted near-infrared imaging field spectrograph OSIRIS at the Keck Observatory. We present the morphology and dynamics of most species detected but focus on the morphology and dynamics of the narrow line region (as traced by emission of [FeII] λ1.644μm), the interplay between plasma ejected from the nucleus (as traced by 21 cm continuum radio data) and hot H2 gas and characterize the detected nuclear HeI$λ2.058 μm absorption feature as a narrow absorption line (NAL) phenomenon.
26 pages, accepted by A&A
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Cited by in corpus (8)
- Fueling AGN II: Spatially Resolved Molecular Inflows and Outflows
- The Cepheid Distance to the Seyfert 1 Galaxy NGC 4151
- The Keck/OSIRIS Nearby AGN Survey (KONA) I. The Nuclear K-band Properties of Nearby AGN
- Variability of the coronal line region in NGC 4151
- A SINFONI view of the nuclear activity and circum-nuclear star formation in NGC 4303
- Young Star Clusters In The Circumnuclear Region Of NGC 2110
- NIR imaging spectroscopy of the inner few arcseconds of NGC 4151 with OSIRIS at Keck
- Physical properties and the variability mechanism of the He I outflow in NGC 4151