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25 April 2024
 
  » arxiv » astro-ph/0205444

 Article overview



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
AffiliationDepartment 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
AbstractUsing 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
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