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

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

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aspc..289..341c&link_type=abstract

The Proceedings of the IAU 8th Asian-Pacific Regional Meeting, Volume I, held 2-5 July 2002 at National Center of Sciences, Hito

Astronomy and Astrophysics

Astronomy

Scientific paper

The distribution of line luminosity L_Hβ of 23 BL Lac objects suggests a bimodal nature. We found that standard thin disks are probably in the sources with L_Hβ > 10^41 erg s^-1. For the sources with L_Hβ < 10 ^41 erg s^-1, the accretion flows have transited from the standard^ thin disk type to the ADAF type. The results support the evolutionary sequence of blazars as being: FSRQ -> LBL -> HBL.

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