Ultraviolet imaging of the AGN+starburst galaxy NGC 1068

Details Ultraviolet imaging of the AGN+starburst galaxy NGC 1068 Ultraviolet imaging of the AGN+starburst galaxy NGC 1068

Aug 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...430..545n&link_type=abstract

The Astrophysical Journal, vol. 430, no. 2, pt. 1, p. 545-549

Astronomy and Astrophysics

Astronomy

33

Active Galactic Nuclei, Disk Galaxies, Emission Spectra, Galactic Halos, Seyfert Galaxies, Starburst Galaxies, Ultraviolet Emission, Cosmology, Galactic Evolution, Luminosity, Ultraviolet Astronomy, Ultraviolet Telescopes

Scientific paper

Images of the Seyfert 2 galaxy NGC 1068 were obtained at two ultraviolet wavelengths by the Ultraviolet Imaging Telescope (UIT). These data represent the first detailed UV imagery of a composite (active galactic nucleus + starburst) disk galaxy. NGC 1068 contains multiple components at UV wavelengths: the central active galactic nucleus; a population of very luminous starburst knots; a bright oval inner disk; and a fainter, more circular halo. The most luminous knot, which is located approximately 750 pc from the nucleus at PA 315 deg, is approximately 80 times the luminosity of 30 Doradus and gives NGC 1068 a 'double nucleus' appearance in the UV. Significant extended emission is observed throughout the disk, unlike other disk galaxies so far observed in the UV. The radial brightness profile in both UV bandpasses generally follows an exponential decline to approximately 5 kpc. A faint halo extending to approximately 13 kpc is likely to be a galaxian-sized reflection nebula where ambient dust scatters the intense UV continuum from the inner galaxy. UV colors show a striking asymmetric morphology, which is correlated with the observed molecular CO emission.

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