Chandra observation of supernova remnant G54.1+0.3: A close cousin of the Crab Nebula
文献类型:期刊论文
作者 | Lu FJ(卢方军)![]() ![]() ![]() ![]() |
刊名 | ASTROPHYSICAL JOURNAL
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出版日期 | 2002 |
卷号 | 568期号:1页码:L49-L52 |
关键词 | ISM : individual (G54.1+0.3) ISM : jets and outflows stars : neutron supernova remnants X-rays : ISM |
通讯作者 | Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA ; Chinese Acad Sci, Inst High Energy Phys, Lab Cosm Ray & High Energy Astrophys, Beijing 100039, Peoples R China ; Max Planck Inst Extraterr Phys, D-85741 Garching, Germany ; Ctr Etud Saclay, DAPNIA, DSM, Serv Astrophys, F-91191 Gif Sur Yvette, France |
英文摘要 | We present a Chandra Advanced CCD Imaging Spectrometer observation of supernova remnant G54.1+0.3. This supernova remnant is resolved into several distinct X-ray-emitting components: a central bright pointlike source (CXOU J193030.13+185214.1), a surrounding ring, bipolar elongations, plus low surface brightness diffuse emission. The spectra of these components are all well described by power-law models; the spectral index steepens with increasing distance from the pointlike source. We find no evidence for any thermal plasma emission that would correspond to shocked interstellar medium or ejecta. The observed morphological and spectral characteristics suggest that G54.1+0.3 is the closest "cousin" of the Crab Nebula-a pulsar wind nebula driven by a combination of equatorial and polar outflows from the putative pulsar represented by the pointlike X-ray source. |
学科主题 | Astronomy & Astrophysics |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
原文出处 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000174438300012 |
源URL | [http://ir.ihep.ac.cn/handle/311005/240277] ![]() |
专题 | 高能物理研究所_粒子天体物理中心 |
作者单位 | 中国科学院高能物理研究所 |
推荐引用方式 GB/T 7714 | Lu FJ,Lu, FJ,Wang, QD,et al. Chandra observation of supernova remnant G54.1+0.3: A close cousin of the Crab Nebula[J]. ASTROPHYSICAL JOURNAL,2002,568(1):L49-L52. |
APA | 卢方军.,Lu, FJ.,Wang, QD.,Aschenbach, B.,Durouchoux, P.,...&宋黎明.(2002).Chandra observation of supernova remnant G54.1+0.3: A close cousin of the Crab Nebula.ASTROPHYSICAL JOURNAL,568(1),L49-L52. |
MLA | 卢方军,et al."Chandra observation of supernova remnant G54.1+0.3: A close cousin of the Crab Nebula".ASTROPHYSICAL JOURNAL 568.1(2002):L49-L52. |
入库方式: OAI收割
来源:高能物理研究所
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