Modeling the Strongest Silicate Emission Features of Local Type 1 AGNs
We measure the 10 and 18 μm silicate features in a sample of 67 local (z < 0.1) type 1 active galactic nuclei (AGN) with available Spitzer spectra dominated by nonstellar processes. We find that the 10 μm silicate feature peaks at ${10.3}_{-0.9}^{+0.7}\,\mu {\rm{m}}$ with a strength (Si p = ln f p(spectrum)/f p(continuum)) of ${0.11}_{-0.36}^{+0.15
Martínez-Paredes, M. et al.
Advertised on:
2
2020