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Jet Properties of GeV-selected Radio-loud Narrow-line Seyfert 1 Galaxies and Possible Connection to Their Disk and Corona

  • Authors: Xiao-Na Sun, Jin Zhang, Da-Bin Lin, Zi-Wei Xue, En-Wei Liang, and Shuang-Nan Zhang

Sun et al. 2015 The Astrophysical Journal 798 43.

  • Provider: AAS Journals

Caption: Figure 6.

Jet total power (a) and jet radiation power (b) as a function of the accretion disk luminosity. The solid lines are the equality lines. The blazar data (opened symbols) and the fitting lines (dashed lines) for FSRQs are taken from Ghisellini et al. (2010). The open symbols with different colors correspond to blazars with different γ-ray observed luminosities: stars for Lγ > 1048.5, squares for 1047.5 < Lγ < 1048.5, triangles for 1046.5 < Lγ < 1047.5, circles for 1045.5 < Lγ < 1046.5, and diamonds for Lγ < 1045.5.

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