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The revised distance of supernova remnant G15.4+0.1
Su, Hong-Quan1,2,3; Zhang, Meng-Fei1,2; Zhu, Hui1; Wu, Dan1,4
2017-09-01
Source PublicationRESEARCH IN ASTRONOMY AND ASTROPHYSICS
Volume17Issue:10
AbstractWe measure the distance to the supernova remnant G15.4+0.1 which is likely associated with TeV source HESS J1818-154. We build the neutral hydrogen (HI) absorption and (CO)-C-13 spectra for supernova remnant G15.4+0.1 by employing data from the Southern Galactic Plane Survey (SGPS) and the HI/OH/Recombination line survey (THOR). The maximum absorption velocity of about 140 km s(-1) constrains the lower limit of its distance to about 8.0 kpc. Further, the fact that the HI emission feature at about 95 km s(-1) seems to have no corresponding absorption suggests that G15.4+0.1 likely has an upper limit for distance of about 10.5 kpc. The (CO)-C-13 spectrum for the remnant supports our measurement. The new distance provides revised parameters on its associated pulsar wind nebula and TeV source.
SubtypeArticle
KeywordIsm: Supernova Remnants Methods: Data Analysis Stars: Distances
WOS HeadingsScience & Technology ; Physical Sciences
Funding OrganizationNational Natural Science Foundation of China(11473038 ; National Natural Science Foundation of China(11473038 ; 11273025) ; 11273025) ; National Natural Science Foundation of China(11473038 ; National Natural Science Foundation of China(11473038 ; 11273025) ; 11273025)
DOI10.1088/1674-4527/17/10/109
WOS KeywordGALACTIC PLANE SURVEY
Indexed BySCI
Language英语
Funding OrganizationNational Natural Science Foundation of China(11473038 ; National Natural Science Foundation of China(11473038 ; 11273025) ; 11273025) ; National Natural Science Foundation of China(11473038 ; National Natural Science Foundation of China(11473038 ; 11273025) ; 11273025)
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000415007500010
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/20208
Collection光学天文研究部
Affiliation1.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China
2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
3.Curtin Univ, Int Ctr Radio Astron Res, Bentley, WA 6102, Australia
4.Beijing Normal Univ, Coll Informat Sci & Technol, Beijing 100875, Peoples R China
Recommended Citation
GB/T 7714
Su, Hong-Quan,Zhang, Meng-Fei,Zhu, Hui,et al. The revised distance of supernova remnant G15.4+0.1[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2017,17(10).
APA Su, Hong-Quan,Zhang, Meng-Fei,Zhu, Hui,&Wu, Dan.(2017).The revised distance of supernova remnant G15.4+0.1.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,17(10).
MLA Su, Hong-Quan,et al."The revised distance of supernova remnant G15.4+0.1".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 17.10(2017).
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