论文

论文

Theoretical sigma-D relations for shell-type galactic supernova remnants
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论文题目: Theoretical sigma-D relations for shell-type galactic supernova remnants
论文题目英文:
作者: Hu, Ya-Peng; Zeng, Hong-An; Fang, Jun; Hou, Jun-Peng; Xu, Jian-Wen
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刊物名称: JOURNAL OF ASTROPHYSICS AND ASTRONOMY
: 2019
: 40
: 1
: 7
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摘要: 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 adiabatic phase, 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 1GHz. 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.
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