中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Distance and evolutionary state of the supernova remnant G18.1-0.1

文献类型:期刊论文

作者Leahy, Denis1; Green, Kaylie1; Tian, Wenwu2
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2014-02-01
卷号438期号:2页码:1813-1819
关键词ISM: individual objects: G18.1-0.1 ISM: supernova remnants radio lines: ISM X-rays: ISM
英文摘要We analyse radio and X-ray observations of the supernova remnant (SNR) G18.1-0.1 and the overlapping and surrounding HII regions. The HI absorption spectra yield a new distance of 5.6 kpc to G18.1-0.1 and confirm previous distance estimates for the surrounding HII regions. All of the HII regions are significantly closer (d = 2.9 to 4.1 kpc) than SNR G18.1-0.1, so we conclude that they are not physically associated. Chandra archival X-ray observations of G18.1-0.1 show extended shell-type X-ray emission from the SNR. The X-ray spectrum is used to determine that the SNR is in the Sedov adiabatic expansion phase. G18.1-0.1 is similar or equal to 8.9 pc radius, middle-aged (5 kyr), expanding in normal density interstellar medium (similar or equal to 0.6 cm(-3)) and has a low explosion energy (similar or equal to 2.5 x 10(50) erg).
收录类别SCI
语种英语
WOS记录号WOS:000330955900068
源URL[http://ir.bao.ac.cn/handle/114a11/6502]  
专题国家天文台_光学天文研究部
作者单位1.Univ Calgary, Calgary, AB T2N 1N4, Canada
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
推荐引用方式
GB/T 7714
Leahy, Denis,Green, Kaylie,Tian, Wenwu. Distance and evolutionary state of the supernova remnant G18.1-0.1[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2014,438(2):1813-1819.
APA Leahy, Denis,Green, Kaylie,&Tian, Wenwu.(2014).Distance and evolutionary state of the supernova remnant G18.1-0.1.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,438(2),1813-1819.
MLA Leahy, Denis,et al."Distance and evolutionary state of the supernova remnant G18.1-0.1".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 438.2(2014):1813-1819.

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来源:国家天文台

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