Fig. 2 from Evidence for the Evolutionary Sequence of Blazars: Different Types of Accretion Flows in BL Lacertae Objects

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Evidence for the Evolutionary Sequence of Blazars: Different Types of Accretion Flows in BL Lacertae Objects

Authors: Xinwu Cao

Cao 2002 The Astrophysical Journal Letters 570 L13.

Provider: AAS Journals

Caption: Fig. 2.

Maximal optical luminosity of ADAFs at 4861 Å as functions of black hole mass for different values of α: ﹩\alpha =0.1﹩ (dashed line), 0.3 (solid line), and 1 (dotted line).

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