NASA Technical Reports Server (NTRS) 20140011111: Suzaku View Of The Swift/BAT Active Galactic Nuclei. V. Torus Structure Of Two Luminous Radio-Loud Active Galactic Nuclei (3C 206 And PKS 0707-35) - Info and Reading Options
By NASA Technical Reports Server (NTRS)
"NASA Technical Reports Server (NTRS) 20140011111: Suzaku View Of The Swift/BAT Active Galactic Nuclei. V. Torus Structure Of Two Luminous Radio-Loud Active Galactic Nuclei (3C 206 And PKS 0707-35)" and the language of the book is English.
“NASA Technical Reports Server (NTRS) 20140011111: Suzaku View Of The Swift/BAT Active Galactic Nuclei. V. Torus Structure Of Two Luminous Radio-Loud Active Galactic Nuclei (3C 206 And PKS 0707-35)” Metadata:
- Title: ➤ NASA Technical Reports Server (NTRS) 20140011111: Suzaku View Of The Swift/BAT Active Galactic Nuclei. V. Torus Structure Of Two Luminous Radio-Loud Active Galactic Nuclei (3C 206 And PKS 0707-35)
- Author: ➤ NASA Technical Reports Server (NTRS)
- Language: English
Edition Identifiers:
- Internet Archive ID: NASA_NTRS_Archive_20140011111
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"NASA Technical Reports Server (NTRS) 20140011111: Suzaku View Of The Swift/BAT Active Galactic Nuclei. V. Torus Structure Of Two Luminous Radio-Loud Active Galactic Nuclei (3C 206 And PKS 0707-35)" Description:
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We present the results from broadband X-ray spectral analysis of 3C 206 and PKS 0707-35 with Suzaku and Swift/BAT, two of the most luminous unobscured and obscured radio-loud active galactic nuclei (AGNs) with hard X-ray luminosities of 10(sup 45.5) erg per second and 10(sup 44.9) erg per second (14-195 keV), respectively. Based on the radio core luminosity, we estimate that the X-ray spectrum of 3C 206 contains a significant (~60% in the 14-195 keV band) contribution from the jet, while it is negligible in PKS 0707-35.We can successfully model the spectra with the jet component (for 3C 206), the transmitted emission, and two reflection components from the torus and the accretion disk. The reflection strengths from the torus are found to be R(sub torus)(=Omega/2pi) = 0.29 +/- 0.18 and 0.41 +/- 0.18 for 3C 206 and PKS 0707-35, respectively, which are smaller than those in typical Seyfert galaxies. Utilizing the torus model by Ikeda et al., we quantify the relation between the half-opening angle of a torus (theta(sub oa)) and the equivalent width of an iron-K line. The observed equivalent width of 3C 206, less than 71 eV, constrains the column density in the equatorial plane to N(sup eq)(sub H) lesst han 10(sup 23) per square centimeter, or the half-opening angle to theta(sub oa) greater than 80 deg. if N(sup eq)(sub H) = 10(sup 24) per square centimeter is assumed. That of PKS 0707-35, 72 +/- 36 eV, is consistent with N(sup eq)(sub H) ~ 10(sup 23) per square centimeter. Our results suggest that the tori in luminous radio-loud AGNs are only poorly developed. The trend is similar to that seen in radio-quiet AGNs, implying that the torus structure is not different between AGNs with jets and without jets.
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