Low Resolution IRS Spectra of Nearby Seyfert Galaxies

Details Low Resolution IRS Spectra of Nearby Seyfert Galaxies Low Resolution IRS Spectra of Nearby Seyfert Galaxies

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..381..409g&link_type=abstract

The Second Annual Spitzer Science Center Conference: Infrared Diagnostics of Galaxy Evolution. ASP Conference Series, Vol. 381,

Astronomy and Astrophysics

Astronomy

Scientific paper

We have obtained low-resolution spectra of 42 nearby Seyfert Active Galactic Nuclei. The AGNs were chosen to have a broad range of X-ray determined Hydrogen column densities from Compton thin to Compton thick. The spectral energy distributions are broadly consistent with higher column densities showing greater short wavelength absorption than lower column densities.

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