The unification of RBLs with XBLs

Details The unification of RBLs with XBLs The unification of RBLs with XBLs

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ap%26ss.318..169b&link_type=abstract

Astrophysics and Space Science, Volume 318, Issue 3-4, pp. 169-180

Astronomy and Astrophysics

Astrophysics

1

Galaxies, Bl Lacertae Objects, Light Curve, Redshift, Mass Of Black Hole, Flux

Scientific paper

Many astronomers have discussed the property of BL Lacertae objects, including the variation of spectrum, the correlation of multi-wave bands and the property of polarization, which could give good information for studying intrinsic correlation of components and position of BL Lacertae objects. In the paper, we investigated the properties of RBLs and XBLs and RBLs/XBLs (these objects can also be found by radio survey as by X-ray survey). Firstly, we collected the light curve of 28 BL Lacertae objects, and gained their short timescales by Structure Function (SF). Secondly, we analyzed the distribution of the short timescales of some BL Lacertae objects, including 28 objects’ timescales calculated by SF, as well as the distribution of the redshift and the black hole mass and the flux densities of the multi-wavebands (radio, near-infrared, optical and Gamma-ray). Based on statistical analysis, the result of the paper support the unification model of RBLs and XBLs.

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