Fan Junhui, Feng Xianchan, Su Chengyue. The Observation Properties of Radio-Selected BLLac Objects (RBLs)—(Ⅱ)[J]. Astronomical Techniques and Instruments, 1999, (2): 1-16.
Citation:
Fan Junhui, Feng Xianchan, Su Chengyue. The Observation Properties of Radio-Selected BLLac Objects (RBLs)—(Ⅱ)[J]. Astronomical Techniques and Instruments, 1999, (2): 1-16.
Fan Junhui, Feng Xianchan, Su Chengyue. The Observation Properties of Radio-Selected BLLac Objects (RBLs)—(Ⅱ)[J]. Astronomical Techniques and Instruments, 1999, (2): 1-16.
Citation:
Fan Junhui, Feng Xianchan, Su Chengyue. The Observation Properties of Radio-Selected BLLac Objects (RBLs)—(Ⅱ)[J]. Astronomical Techniques and Instruments, 1999, (2): 1-16.
The Observation Properties of Radio-Selected BLLac Objects (RBLs)—(Ⅱ)
In this paper, object swhich have been classified as BLLac objects have been compiled as a supplement to our previous paper (Fan&Lin 1996). The relation between large optical variation and largest optical polarization has been explained in the frame of relativistic beaming model.
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