Influence of the active nucleus on the multiphase interstellar medium in NGC 1068

Details Influence of the active nucleus on the multiphase interstellar medium in NGC 1068 Influence of the active nucleus on the multiphase interstellar medium in NGC 1068

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993egte.conf..305b&link_type=abstract

In NASA. Ames Research Center, The Evolution of Galaxies and Their Environment p 305-306 (SEE N93-26706 10-90)

Computer Science

Active Galactic Nuclei, Interstellar Matter, Seyfert Galaxies, H Ii Regions, Interferometry, Luminosity, Oxygen Spectra, Photoexcitation, Rosat Mission, Spectrophotometry

Scientific paper

The luminous spiral NGC 1068 has now been imaged from x-ray to radio wavelengths at comparably high resolution (approximately less than 5 in. FWHM). The bolometric luminosity of this well-known Seyfert is shared almost equally between the active nucleus and an extended 'starburst' disk. In an ongoing study, we are investigating the relative importance of the nucleus and the disk in powering the wide range of energetic activity observed throughout the galaxy. Our detailed analysis brings together a wealth of data: ROSAT HRI observations, VLA lambda lambda 6-20 cu cm and OVRO interferometry, lambda lambda 0.4-10.8 micron imaging, and Fabry-Perot spectrophotometry.

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