Chandra observation of PWN G16.73+0.08 in SNR G16.7+0.1
文献类型：期刊论文
| 作者 | Chang, H. -K.1,2; Chung, S. -F.1; Yang, C. -Y.1; Tian, W. W.3,4 |
| 刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
 |
| 出版日期 | 2018-02-01 |
| 卷号 | 474期号:2页码:2607-2611 |
| ISSN号 | 0035-8711 |
| 关键词 | radiation mechanisms: non-thermal stars: neutron pulsars: general ISM: individual objects: G16.7+0.1 ISM: supernova remnants X-rays: individual: G16.73+0.08 |
| DOI | 10.1093/mnras/stx2941 |
| 英文摘要 | We present X-ray observations of pulsar wind nebula (PWN) G16.73+0.08/supernova remnant (SNR) G16.7+0.1 using archival data of Chandra ACIS. The X-ray emission peak location of this PWN is found to be offset by 24 arcsec from the centre of the 1.4-GHz emission of this nebula. The X-ray nebula is elongated in the direction from the X-ray peak to the 1.4-GHz emission centre. This offset suggests that G16.73+0.08 is an evolved PWN interacting with the SNR reverse shock. We identify a point source, CXOJ182058.16-142001.5, near the location of the X-ray peak. The spectrum of the X-ray nebula can be described by an absorbed power law of photon index 0.98(-0.71)(+0.79) and hydrogen column density N-H = 4.99(-2.28)(+2.75) x 10(22) cm(-2). CXO J182058.16 - 142001.5 is likely a pulsar. We estimate its spin-down power to be about 2.6 x 10(36) erg s(-1). Assuming its age at 3000 and 10 000 yr, its dipole magnetic field strength at the polar surface is estimated to be about 4.2 x 10(13) and 1.3 x 10(13) G, respectively. |
| WOS关键词 | PULSAR-WIND NEBULAE ; SUPERNOVA REMNANT ; X-RAY ; SYNCHROTRON NEBULAE ; EMISSION ; G327.1-1.1 ; SPECTRA ; RADIO ; JETS |
| 资助项目 | Ministry of Science and Technology of the Republic of China[MOST 105-2112-M-007-002] ; Ministry of Science and Technology of the Republic of China[MOST 106-2811-M-007-008] |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| 出版者 | OXFORD UNIV PRESS |
| WOS记录号 | WOS:000424343600085 |
| 资助机构 | Ministry of Science and Technology of the Republic of China ; Ministry of Science and Technology of the Republic of China ; Ministry of Science and Technology of the Republic of China ; Ministry of Science and Technology of the Republic of China ; Ministry of Science and Technology of the Republic of China ; Ministry of Science and Technology of the Republic of China ; Ministry of Science and Technology of the Republic of China ; Ministry of Science and Technology of the Republic of China |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/37204]  |
| 专题 | 中国科学院国家天文台 |
| 通讯作者 | Chang, H. -K. |
| 作者单位 | 1.Natl Tsing Hua Univ, Inst Astron, Hsinchu 30013, Taiwan 2.Natl Tsing Hua Univ, Dept Phys, Hsinchu 30013, Taiwan 3.Chinese Acad Sci, Key Lab Opt Astron, Natl Astron Observat, Beijing 100049, Peoples R China 4.Univ Calgary, Dept Phys & Astron, Calgary, AB T2N 1N4, Canada |
| 推荐引用方式 GB/T 7714 | Chang, H. -K.,Chung, S. -F.,Yang, C. -Y.,et al. Chandra observation of PWN G16.73+0.08 in SNR G16.7+0.1[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2018,474(2):2607-2611. |
| APA | Chang, H. -K.,Chung, S. -F.,Yang, C. -Y.,&Tian, W. W..(2018).Chandra observation of PWN G16.73+0.08 in SNR G16.7+0.1.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,474(2),2607-2611. |
| MLA | Chang, H. -K.,et al."Chandra observation of PWN G16.73+0.08 in SNR G16.7+0.1".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 474.2(2018):2607-2611. |
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来源：国家天文台
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