Near-Infrared Emission-Line Spectrum of NGC 1068

Details Near-Infrared Emission-Line Spectrum of NGC 1068 Near-Infrared Emission-Line Spectrum of NGC 1068

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aas...187.5606o&link_type=abstract

American Astronomical Society, 187th AAS Meeting, #56.06; Bulletin of the American Astronomical Society, Vol. 27, p.1367

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Scientific paper

Relative line-flux measurements are given of the Seyfert 2, "hidden-BLR" galaxy NGC 1068 in the near-infrared spectral region lambda lambda 7000 - 10830. They are corrected approximately for extinction in a ``one-layer'' model, and are discussed in terms of ionization and energy-input, particularly in the high-ionization regions in which [Fe XI] lambda7892 and [S VIII] lambda9913 are emitted. The need for new calculations of collision strengths for these and other similar ions is emphasized, based on current quantum-mechanical methods using large numbers of multi-configuration wave functions.

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