Abstract
We present the arcsecond-scale jet structure and related radio properties for a sample of 9 UHBLs selected from Nieppola et al. (2006) with log(ν p e a k /H z)>20. Our preliminary results show that most of the UHBLs have compact structures, and their core dominance parameters are much larger than FR-I radio galaxies, suggesting that beaming may be prevalent in the jets of these sources.
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Acknowledgements
We thank the anonymous referee for insightful comments and constructive suggestions. This work is supported by the 973 Programme (No. 2009CB824800), the NSFC grants (Nos 11163002 and 11073039) and by the Study Abroad Fund from China Scholarship Council (No. [2011]5024).
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Wu, Z., Yang, S. & Gu, M. Arcsecond-Scale Radio Jets of Ultra-High-Energy Synchrotron Peak BL Lacs (UHBLs). J Astrophys Astron 35, 321–323 (2014). https://doi.org/10.1007/s12036-014-9221-0
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DOI: https://doi.org/10.1007/s12036-014-9221-0