8-13 microns spectrophotometry of galaxies. IV - Six more Seyferts and 3C345. V - The nuclei of five spiral galaxies

Astronomy and Astrophysics – Astronomy

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Galactic Nuclei, Infrared Spectra, Quasars, Seyfert Galaxies, Spectrophotometry, Active Galaxies, Astronomical Models, Cosmic Dust, Starburst Galaxies

Scientific paper

The low-resolution spectra of six Seyfert nuclei and the quasar 3C345 are presented, together with four more starburst nuclei spectra observed in a companion study. The spectra were obtained using the UCL LH-cooled grating spectrometer with an array of 25 As:Si photoconductors in a low resolution mode covering a wavelength range of 7.7-13.3 microns. It is shown that the active galaxies are characterized by power law spectra with a tendency for the spectral index to steepen with the progression quasar-Seyfert 1-Seyfert 2 and with silicate absorption in Seyfert 2 galaxies. In contrast, the starburst galaxy spectra are dominated by emission from unidentified dust-associated features and frequently show the fine structure forbidden line of Ne II. The possible origins for the unidentified features in the starburst galaxy spectra are discussed.

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