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所属单位：理学院

发表刊物：JOURNAL OF ASTROPHYSICS AND ASTRONOMY

关键字：Shell-type supernova remnants radiative phase surface brightness sigma-D relation

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.

ISSN号：0250-6335

是否译文：否

发表时间：2019-02-01

合写作者：Zeng, Hong-An,Fang, Jun,Hou, Jun-Peng,Xu, Jian-Wen

通讯作者：胡亚鹏