Image Details

Choose export citation format:

Polycyclic Aromatic Hydrocarbon and Emission Line Ratios in Active Galactic Nuclei and Starburst Galaxies

  • Authors: Dinalva A. Sales, M. G. Pastoriza, and R. Riffel

SALES, PASTORIZA, & RIFFEL 2010 The Astrophysical Journal 725 605.

  • Provider: AAS Journals

Caption: Figure 9.

Diagnostic diagram between an indicator of the hardness of the radiation field and [Ne iii]15.5/[Ne ii]12.8 μm versus EW 7.7 μm (top) and EW 11.3 μm (bottom) PAH emission features. Full triangles are SBs taken from Brandl et al. (2006), and full and empty circles are Sy 1 and Sy 2 of our and Gallimore et al. (2010) sample. Error bars are shown only for the 15 new AGNs; similar errors were found for the remaining objects. The lines represent an exponential regression fitted for the total sample (dotted line) and for the AGN sub-sample (solid line).

Other Images in This Article
Copyright and Terms & Conditions