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A Multiwavelength Study of Narrow‐Line Seyfert 1 Galaxies from the Second Byurakan Survey

  • Authors: J. A. Stepanian, E. Benítez, Y. Krongold, I. Cruz-González, J. A. de Diego, V. Chavushyan, R. Mújica, D. Dultzin-Hacyan, and T. Verdugo

Stepanian et al. 2003 The Astrophysical Journal 588 746.

  • Provider: AAS Journals

Caption: Fig. 5.

Diagram of ﹩f_{\mathrm{X}\,}/ f_{\mathrm{opt}\,}﹩ as a function of ﹩M_{B}﹩ for SBS NLS1s (−﹩19.0> M_{B}> -23.0﹩, ﹩B< 17.5﹩; diamonds; ﹩N=14﹩), added to the diagram of BQX QSOs of Schmidt & Green (1986; squares; −﹩23.0> M_{B}> -30.0﹩, ﹩N=52﹩). Fainter objects (﹩B> 17.5﹩; stars) and upper limits (triangles) are also represented.

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