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A possible explanation of the parallel tracks in kilohertz quasi-periodic oscillations from low-mass-X-ray binaries (vol 479, pg 5049, 2018)
Shi, Chang-Sheng1,3; Zhang, Shuang-Nan2,5,6; Li, Xiang-Dong3,4
2019-10-01
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
Volume489Issue:2Pages:2307-2307
Keywordaccretion: accretion discs X-rays: binaries MHD stars: magnetic fields
DOI10.1093/mnras/stz2369
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000489298100063
PublisherOXFORD UNIV PRESS
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Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/28043
Collection中国科学院国家天文台
Corresponding AuthorShi, Chang-Sheng
Affiliation1.Hainan Univ, Sch Sci, Haikou 570228, Hainan, Peoples R China
2.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China
3.Nanjing Univ, Key Lab Modern Astron & Astrophys, Minist Educ, Nanjing 210093, Jiangsu, Peoples R China
4.Nanjing Univ, Dept Astron, Nanjing 210093, Jiangsu, Peoples R China
5.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
6.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
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Shi, Chang-Sheng,Zhang, Shuang-Nan,Li, Xiang-Dong. A possible explanation of the parallel tracks in kilohertz quasi-periodic oscillations from low-mass-X-ray binaries (vol 479, pg 5049, 2018)[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2019,489(2):2307-2307.
APA Shi, Chang-Sheng,Zhang, Shuang-Nan,&Li, Xiang-Dong.(2019).A possible explanation of the parallel tracks in kilohertz quasi-periodic oscillations from low-mass-X-ray binaries (vol 479, pg 5049, 2018).MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,489(2),2307-2307.
MLA Shi, Chang-Sheng,et al."A possible explanation of the parallel tracks in kilohertz quasi-periodic oscillations from low-mass-X-ray binaries (vol 479, pg 5049, 2018)".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 489.2(2019):2307-2307.
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