Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...131..159p&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 131, no. 1, Feb. 1984, p. 159-168.
Astronomy and Astrophysics
Astronomy
80
Astronomical Models, Astronomical Spectroscopy, Elliptical Galaxies, Galactic Nuclei, Photoionization, Accretion Disks, Active Galactic Nuclei, Active Galaxies, Black Body Radiation, Black Holes (Astronomy), Emission Spectra, Line Spectra, Oxygen Spectra, Ultraviolet Astronomy
Scientific paper
It is shown that the emission line spectrum produced in the active galactic nucleus and the surrounding nebulosity of the elliptical galaxy NGC 1052, which is presently the most compelling candidate for shock-heating excitation, can also be understood in terms of photoionization by a central source of radiation if (1) the ionizing continuum looks like a blackbody of temperature around 8×104K prolonged by a flat soft X-ray continuum, so that a marked break appears around 5 Ryd, and (2) the gas is strongly stratified in the unresolved nucleus, so that the lines arise from several concentric regions with the density ranging from less than 103 cm-3 to at least 107 cm-3. The photoionization hypothesis in NGC 1052 leads to specific predictions concerning (1) the line ratios in and out of the nucleus, (2) the line profiles in the nucleus and (3) the reddening of the lines by dust.
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