O VI Emission in Nuclear Region of NGC 1068

Details O VI Emission in Nuclear Region of NGC 1068 O VI Emission in Nuclear Region of NGC 1068

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1135...52z&link_type=abstract

FUTURE DIRECTIONS IN ULTRAVIOLET SPECTROSCOPY: A Conference Inspired by the Accomplishments of the Far Ultraviolet Spectroscopic

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Quasars, Active Or Peculiar Galaxies, Objects, And Systems, Photoionization Of Atoms And Ions, Astronomical Catalogs, Atlases, Sky Surveys, Databases, Retrieval Systems, Archives, Etc.

Scientific paper

FUSE Spectra of the nuclear region of NGC 1068 find strong OVI emission consisting of a pair of narrow and broad components. There is a gradient in the velocity field for the narrow O VI component of ~200 kms-1 from ~2'' southwest of the nucleus to ~4'' northeast. A similar pattern is also observed with the broad O VI component, with a gradient of ~3000 kms-1. These results are consistent with the HST/STIS findings and suggest a biconical structure in which the velocity field is mainly radial outflow.

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