Theoretical sigma-D relations for shell-type galactic supernova remnants
文献类型：期刊论文
| 作者 | Hu, YP; Zeng, HA; Fang, J1; Hou, JP; Xu, JW |
| 刊名 | JOURNAL OF ASTROPHYSICS AND ASTRONOMY
 |
| 出版日期 | 2019 |
| 卷号 | 40期号:1页码:7 |
| 关键词 | X-RAY OBSERVATIONS COMPACT CENTRAL OBJECT RADIO OBSERVATIONS ROSAT OBSERVATIONS NOVA REMNANTS INTERSTELLAR-MEDIUM EMISSION ACCELERATION DEPENDENCE DISTANCES |
| ISSN号 | 0250-6335 |
| DOI | 10.1007/s12036-019-9574-5 |
| 英文摘要 | 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. |
| 学科主题 | Astronomy & Astrophysics |
| 语种 | 英语 |
| 源URL | [http://ir.itp.ac.cn/handle/311006/23498]  |
| 专题 | 理论物理研究所_理论物理所1978-2010年知识产出 |
| 作者单位 | 1.Chinese Acad Sci, Inst Theoret Phys, Key Lab Frontiers Theoret Phys, Beijing 100080, Peoples R China 2.Yunnan Univ, Dept Astron, Kunming 650091, Yunnan, Peoples R China 3.Nanjing Univ Aeronaut & Astronaut, Coll Sci, Nanjing 210016, Jiangsu, Peoples R China |
| 推荐引用方式 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. |
入库方式： OAI收割
来源：理论物理研究所
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