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Article overview
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Radio Luminosities and Classificatory Criteria of BL Lacertae Objects | D. C. Mei
; L.Zhang
; Z. J. Jiang
; B.Z.Dai
; | Date: |
25 May 2002 | Subject: | astro-ph | Affiliation: | Department of Physics, Yunnan University), L.Zhang (Department of Physics, Yunnan University), Z. J. Jiang (Department of Physics, Yunnan University), B.Z.Dai (Department of Physics, Yunnan University | Abstract: | Using the sample of radio selected BL Lacertae objects (RBLs) and X-ray selected BL Lacertae objects (XBLs) presented by Sambruna et al. (1996), we calculated the luminosities of radio, optical and X-ray of each source and made the statistical analysis among the luminosities at different wave-bands, broad-band spectral indices from radio to X-ray ($alpha_{
m rx}$) and peak frequencies ($
u_p$). Our results are as follows: (i) there is a positive correlation between radio luminosity $L_{
m r}$ and $alpha_{
m rx}$ and a negative correlation between $L_{
m r}$ and $
u_p$. High-energy peak BL Lacs (HBLs) and low-energy peak BL Lacs (LBLs) can be distinguished very well, the dividing lines are probably those of $log {L_{
m r}}=43.25$ (erg/sec) and $alpha_{
m rx}>$(or $leq $)0.75 for $L_{
m r}$ - $alpha_{
m rx}$ plot and those of $log {L_{
m r}}leq 43.25$ (erg/sec) and $log {
u_p}>14.7$ for the $L_{
m r}$ - $
u_p$ plot; (ii) there is a weak positive correlation between optical luminosity $L_o$ and $alpha_{
m rx}$ and a negatively weak correlation between $L_{
m o}$ and $
u_p$; (iii) there is no correlation between X-ray luminosity $L_X$ and $alpha_{
m rx}$ or between $L_X$ and $
u_p$. From our analysis, we find that synchrotron radiation is the main X-ray radiation mechanism for HBLs while inverse Compton scattering for LBLs. | Source: | arXiv, astro-ph/0205444 | Services: | Forum | Review | PDF | Favorites |
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