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Study of FHILs in low luminosity AGNs in the optical spectra

Published online by Cambridge University Press:  25 July 2014

Rafael J. C. Vera ,
Ana M. Rodríguez  and
J. Gregorio Portilla
Rafael J. C. Vera
Affiliation:
Observatorio Astronómico Nacional, Universidad Nacional de Colombia, Carrera 45 No 26-85, Bogotá DC, Colombia email: rjverar@bt.unal.edu.co
Ana M. Rodríguez
Affiliation:
Observatorio Astronómico Nacional, Universidad Nacional de Colombia, Carrera 45 No 26-85, Bogotá DC, Colombia email: anamrodriguezv@unal.edu.co
J. Gregorio Portilla
Affiliation:
Observatorio Astronómico Nacional, Universidad Nacional de Colombia, Carrera 45 No 26-85, Bogotá DC, Colombia email: jgportillab@unal.edu.co
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Abstract

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This work presents the main results from a selection of optical spectra of Seyfert and LINER galaxies taken from the 9th release of the SDSS with detectable coronal emission. A catalogue of 345 Seyfert 1 (Sy1) and Seyfert 2 (Sy2) galaxies with Forbidden High Ionization Lines (FHILs) emission is presented. By analysing their spectra as well as utilising data from the literature we found evidence of anisotropy in optical FHIL emissions between Sy1 and Sy2 galaxies for the following lines: [Ne v] λ3426, [Fe vii] λ6087, [Fe x] λ6374 and [Fe xi] λ7892. Results continue indicating that optical FHILs are not observed in LINER type galaxies.

Keywords

galaxies: active galaxies: Seyfert galaxies: Liner quasars: emission lines quasars: coronal line
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S304: Multiwavelength AGN Surveys and Studies , October 2013 , pp. 24 - 27
Copyright
Copyright © International Astronomical Union 2014 

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