Fig. 1 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. 1.

Optical luminosity of ADAFs at 4861 Å as it varies with accretion rate ﹩\dot{m}﹩ for different black hole masses (﹩\alpha =0.3﹩ and ﹩\beta =0.5﹩ are adopted).

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