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      Permanent link:
      https://www.ias.ac.in/article/fulltext/joaa/040/01/0007

    • Keywords

       

      Shell-type supernova remnants; radiative phase; surface brightness; $\Sigma$-$D$ relation.

    • Abstract

       

      Relations between radio surface brightness ($\Sigma$) and diameter ($D$) of supernova remnants (SNRs) are important in astronomy. In this paper, following the work Duric and Seaquist (ApJ 301:308, 1986) at adiabaticphase, we carefully investigate shell-type supernova remnants at radiative phase, and obtain theoretical $\Sigma$-$D$ relation at radiative phase of shell-type supernova remnants at 1 GHz. By using these theoretical $\Sigma$-$D$ relations at adiabatic phase and radiative phase, we also roughly determine phases of some supernova remnant from observation data.

    • Author Affiliations

       

      YA-PENG HU1 2 HONG-AN ZENG1 JUN FANG3 JUN-PENG HOU1 JIAN-WEN XU2

      1. College of Science, Nanjing University of Aeronautics and Astronautics, Nanjing 210016, China.
      2. Key Laboratory of Frontiers in Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100080, China.
      3. Department of Astronomy, Yunnan University, Kunming 650091, China.
    • Dates

       
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