中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
astudyonthecorrelationsbetweenthetwinkhzqpofrequenciesinscox1

文献类型:期刊论文

作者Yin Hongxing2; Zhang Chengmin2; Zhao Yongheng2; Song Liming1; Zhang Fan1
刊名chinesejournalofastronomyandastrophysics
出版日期2005
卷号5期号:6页码:595
ISSN号1009-9271
英文摘要For the bright neutron star low-mass X-ray binary Sco X-1, we analyzed all updated frequencies of the twin kilohertz quasi-periodic oscillations (kHz QPOs), their correlations and distributions. We found that the frequency separation of the kHz QPO peaks appears not to be a constant, rather, it decreases with increasing inferred mass accretion rate. We show that the currently available data of Sco X-1 by Rossi X-ray Timing Explorer are inconsistent with the proposals of the beat model that the frequency separation is a constant. Our conclusions are consistent with those of some previous researchers and we discuss further implications for the kilohertz QPO models.
语种英语
源URL[http://ir.bao.ac.cn/handle/114a11/44430]  
专题光学部_LAMOST运行和发展中心
作者单位1.中国科学院高能物理研究所
2.中国科学院国家天文台
推荐引用方式
GB/T 7714
Yin Hongxing,Zhang Chengmin,Zhao Yongheng,et al. astudyonthecorrelationsbetweenthetwinkhzqpofrequenciesinscox1[J]. chinesejournalofastronomyandastrophysics,2005,5(6):595.
APA Yin Hongxing,Zhang Chengmin,Zhao Yongheng,Song Liming,&Zhang Fan.(2005).astudyonthecorrelationsbetweenthetwinkhzqpofrequenciesinscox1.chinesejournalofastronomyandastrophysics,5(6),595.
MLA Yin Hongxing,et al."astudyonthecorrelationsbetweenthetwinkhzqpofrequenciesinscox1".chinesejournalofastronomyandastrophysics 5.6(2005):595.

入库方式: OAI收割

来源:国家天文台

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