The composite UV to far-IR spectrum of NGC 1068: modeling the ionic and molecular emission

Details The composite UV to far-IR spectrum of NGC 1068: modeling the ionic and molecular emission The composite UV to far-IR spectrum of NGC 1068: modeling the ionic and molecular emission

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.577..329s&link_type=abstract

In: Proceedings of the dusty and molecular universe: a prelude to Herschel and ALMA, 27-29 October 2004, Paris, France. Ed. by A

Computer Science

Galaxies: Individual (Ngc 1068), Galaxies: Active, Nuclei, Seyfert, Emission Lines, Starburst

Scientific paper

The multiwavelenth 0.2-200 μm ionic emission line spectrum of the prototypical Seyfert 2 galaxy NGC 1068 is modeled using a two component AGN plus starburst photoionization model. The agreement between the composite model and the observed spectrum is very satisfactory. Far-infrared OH emission lines have also been detected in NGC 1068 with the ISO-LWS spectrometer. This emission has been modeled using a radiative transfer code for both the continuum and the lines. The origin of these lines from both the nucleus and the extended starburst is investigated and discussed.

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