Theoretical sigma-D relations for shell-type galactic supernova remnants

doi:10.1007/s12036-019-9574-5

ITP OpenIR > SCI期刊论文

	Hu, YP ; Zeng, HA ; Fang, J 2; Hou, JP ; Xu, JW
	Theoretical sigma-D relations for shell-type galactic supernova remnants
Source Publication	JOURNAL OF ASTROPHYSICS AND ASTRONOMY
Language	英语
Keyword	X-RAY OBSERVATIONS COMPACT CENTRAL OBJECT RADIO OBSERVATIONS ROSAT OBSERVATIONS NOVA REMNANTS INTERSTELLAR-MEDIUM EMISSION ACCELERATION DEPENDENCE DISTANCES
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 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.
	2019
ISSN	0250-6335
Volume	40 Issue:1 Pages:7
Subject Area	Astronomy & Astrophysics
MOST Discipline Catalogue	Astronomy & Astrophysics
DOI	10.1007/s12036-019-9574-5
Indexed By	SCIE
Citation statistics
Document Type	期刊论文
Identifier	http://ir.itp.ac.cn/handle/311006/23498
Collection	SCI期刊论文
Affiliation	1.Nanjing Univ Aeronaut & Astronaut, Coll Sci, Nanjing 210016, Jiangsu, Peoples R China 2.Chinese Acad Sci, Inst Theoret Phys, Key Lab Frontiers Theoret Phys, Beijing 100080, Peoples R China 3.Yunnan Univ, Dept Astron, Kunming 650091, Yunnan, Peoples R China
Recommended Citation GB/T 7714	Hu, YP,Zeng, HA,Fang, J,et al. Theoretical sigma-D relations for shell-type galactic supernova remnants[J]. JOURNAL OF ASTROPHYSICS AND ASTRONOMY,2019,40(1):7.
APA	Hu, YP,Zeng, HA,Fang, J,Hou, JP,&Xu, JW.(2019).Theoretical sigma-D relations for shell-type galactic supernova remnants.JOURNAL OF ASTROPHYSICS AND ASTRONOMY,40(1),7.
MLA	Hu, YP,et al."Theoretical sigma-D relations for shell-type galactic supernova remnants".JOURNAL OF ASTROPHYSICS AND ASTRONOMY 40.1(2019):7.

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