1. Home
    2. Journals
    3. Journal of Astrophysics and Astronomy
    4. Volume 35
    5. Issue 3

    • Multi-Wave Luminosity of High-Synchrotron-Peaked TeV BL Lacs Detected by Fermi LAT

      Dingrong Xiong Xiong Zhang Yonggang Zheng

      Part II: Blazar Observations in Infrared and Optical Volume 35 Issue 3 September 2014 pp 237-240

    • Fulltext

       

        Click here to view fulltext PDF


      Permanent link:
      https://www.ias.ac.in/article/fulltext/joaa/035/03/0237-0240

    • Keywords

       

      BL Lacertae objects: general; gamma rays: observations; radiation mechanisms: nonthermal.

    • Abstract

       

      We have studied the correlations between luminosities (𝐿R, 𝐿IR, 𝐿𝛾) in the radio, near-infrared and 𝛾-ray wave bands for HSP TeV BL Lacs. The results show that there are significant intrinsic correlations between 𝐿R and 𝐿𝛾 and between 𝐿IR and 𝐿𝛾 in all states (high/average/low), and suggest that for HSP TeV BL Lacs, the Synchrotron Self-Compton radiation (SSC) is the main mechanism of high energy 𝛾-ray emission, and the inverse Compton scattering of circum-nuclear dust is likely to be an important complementary mechanism.

    • Author Affiliations

       

      Dingrong Xiong1 Xiong Zhang1 Yonggang Zheng1

      1. Department of Physics, Yunnan Normal University, 650 500 Kunming, China.

    • Dates

       
      Published
      September 2014

  • Journal of Astrophysics and Astronomy | News

    • Continuous Article Publication

      Posted on January 27, 2016

      Since January 2016, the Journal of Astrophysics and Astronomy has moved to Continuous Article Publishing (CAP) mode. This means that each accepted article is being published immediately online with DOI and article citation ID with starting page number 1. Articles are also visible in Web of Science immediately. All these have helped shorten the publication time and have improved the visibility of the articles.

    • Editorial Note on Continuous Article Publication

      Posted on July 25, 2019

      Click here for Editorial Note on CAP Mode

© 2017-2019 Indian Academy of Sciences, Bengaluru.

Contact | Site index