中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
首页
机构
成果
学者
登录
注册
登陆
×
验证码:
换一张
忘记密码?
记住我
×
校外用户登录
CAS IR Grid
机构
高能物理研究所 [7]
新疆天文台 [3]
国家天文台 [1]
采集方式
OAI收割 [11]
内容类型
期刊论文 [10]
学位论文 [1]
发表日期
2021 [1]
2019 [1]
2011 [2]
2010 [5]
2000 [2]
学科主题
Astronomy ... [2]
Physics [2]
致密天体、高能和基础... [2]
筛选
浏览/检索结果:
共11条,第1-10条
帮助
条数/页:
5
10
15
20
25
30
35
40
45
50
55
60
65
70
75
80
85
90
95
100
排序方式:
请选择
题名升序
题名降序
发表日期升序
发表日期降序
提交时间升序
提交时间降序
作者升序
作者降序
Synchronous X-ray/Optical QPOs from the Black Hole LMXB MAXI J1820+070
期刊论文
OAI收割
Monthly Notices of the Royal Astronomical Society, 2021
作者:
HXMT
  |  
收藏
  |  
浏览/下载:59/0
  |  
提交时间:2022/02/08
black hole physics
Low Mass X-ray Binaries
accretion
accretion
discs
stars: individual (MAXI J1820+070)
Astrophysics - High Energy
Astrophysical Phenomena
Abstract: We present high-speed optical photometry from SAAO and SALT on the black hole LMXB MAXI J1820+070 (ASSASN-18ey), some of it simultaneous with NICER, Swift and Insight-HXMT X-ray coverage. We detect optical Quasi-Periodic Oscillations (QPOs) that move to higher frequencies as the outburst progresses, tracking both the frequency and evolution of similar X-ray QPOs previously reported. Correlated X-ray/optical data reveal a complex pattern of lags, including an anti-correlation and a sub-second lag that evolve over the first few weeks of outburst. They also show correlated components separated by a lag equal to the QPO period roughly centered on zero lag, implying that the inter-band variability is strongly and consistently affected by these QPOs at a constant phase lag of roughly ±Ю The synchronisation of X-ray and optical QPOs indicates that they must be produced in regions physically very close to each other
we thus propose that they can be explained by a precessing jet model, based on analogies with V404 Cyg and MAXI J1348-630.
Timing analysis of Swift J1658.2-4242's outburst in 2018 with Insight-HXMT, NICER and AstroSat
期刊论文
OAI收割
Journal of High Energy Astrophysics, 2019, 卷号: 24, 页码: 30-40
作者:
HXMT
  |  
收藏
  |  
浏览/下载:61/0
  |  
提交时间:2022/02/08
Accretion
accretion disks
Black hole physics
X-rays: binaries:
Swift J1658.2-4242
Astrophysics - High Energy Astrophysical Phenomena
Abstract: We present the observational results from a detailed timing analysis of the black hole candidate Swift J1658.2-4242 during its 2018 outburst with the observations of Hard X-ray Modulation Telescope (Insight-HXMT), Neutron Star Interior Composition Explorer (NICER) and AstroSat in 0.1-250 keV. The evolution of intensity, hardness and integrated fractional root mean square (rms) observed by Insight-HXMT and NICER are presented in this paper. Type-C quasi-periodic oscillations (QPOs) observed by NICER (0.8-3.5 Hz) and Insight-HXMT (1-1.6 Hz) are also reported in this work. The features of the QPOs are analyzed with an energy range of 0.5-50 keV. The relations between QPO frequency and other characteristics such as intensity, hardness and QPO rms are carefully studied. The timing and spectral properties indicate that Swift J1658.2-4242 is a black hole binary system. Besides, the rms spectra of the source calculated from the simultaneous observation of Insight-HXMT, NICER and AstroSat support the Lense-Thirring origin of the QPOs. The relation between QPO phase lag and the centroid frequency of Swift J1658.2-4242 reveals a near zero constant when < 4Hz and a soft phase lag at 6.68 Hz. This independence follows the same trend as the high inclination galactic black hole binaries such as MAXI J1659-152.
GRS 1915+105 QPO 特性与光子能量关系研究
学位论文
OAI收割
硕士: 中国科学院研究生院, 2011
作者:
鄢淑平
收藏
  |  
浏览/下载:50/0
  |  
提交时间:2013/03/14
吸积
吸积盘
黑洞物理
GRS 1915+105
QPO
中子星X射线双星中kHz QPO现象的理论解释
期刊论文
OAI收割
天文学进展, 2011, 期号: 3, 页码: 277-290
作者:
王静
;
张承民
;
尹红星
;
宋黎明
;
屈进禄
收藏
  |  
浏览/下载:19/0
  |  
提交时间:2015/12/15
X射线双星
吸积
中子星
千赫兹准周期振荡(kHz QPO)
The emission positions of kHz QPOs and Kerr spacetime influence
期刊论文
OAI收割
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2010, 卷号: 53, 期号: Suppl. 1, 页码: 114-116
作者:
Zhang ChengMin
;
Wei YingChun
;
Yin HongXing
;
Zhao YongHeng
;
Lei YaJuan
收藏
  |  
浏览/下载:26/0
  |  
提交时间:2015/08/25
kHz QPO
neutron star
low-mass X-ray binaries
The time lag spectrum of Cir X-1 on its normal branch
期刊论文
OAI收割
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2010, 卷号: 53, 期号: 增刊1, 页码: 60-63
作者:
Qu JinLu
;
Lu Yu
;
Ding GuoQiang
;
Zhang Fan
;
Lei YaJuan
收藏
  |  
浏览/下载:23/0
  |  
提交时间:2013/03/06
Cir X-1
temporal variability
QPO
time lag
The time lag spectrum of Cir X-1 on its normal branch
期刊论文
OAI收割
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2010, 卷号: 53, 期号: 1, 页码: #REF!
作者:
Qu JL(屈进禄)
;
Lu Y(卢宇)
;
Zhang F(张帆)
;
Lei YJ(雷亚娟)
;
Li ZB(李志兵)
收藏
  |  
浏览/下载:33/0
  |  
提交时间:2016/04/11
Cir X-1
temporal variability
QPO
time lag
The emission positions of kHz QPOs and Kerr spacetime influence
期刊论文
OAI收割
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2010, 卷号: 53, 期号: 1, 页码: #REF!
作者:
Zhang, CM
;
Wei, YC
;
Yin, HX
;
Zhao, YH
;
Lei, YJ
收藏
  |  
浏览/下载:27/0
  |  
提交时间:2016/04/12
kHz QPO
neutron star
low-mass X-ray binaries
The emission positions of kHz QPOs and Kerr spacetime influence
期刊论文
OAI收割
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2010, 卷号: 53, 页码: 114-116
作者:
Zhang ChengMin
;
Wei YingChun
;
Yin HongXing
;
Zhao YongHeng
;
Lei YaJuan
收藏
  |  
浏览/下载:27/0
  |  
提交时间:2017/04/19
kHz QPO
neutron star
low-mass X-ray binaries
Correlation between the kilohertz quasi-periodic oscillation and energy spectrum of Aql X-1
期刊论文
OAI收割
CHINESE ASTRONOMY AND ASTROPHYSICS, 2000, 卷号: 24, 期号: 2, 页码: #REF!
作者:
Qu JL(屈进禄)
;
Yu WF(余文飞)
;
Li TB(李惕碚)
;
Qu, JL
;
Yu, WF
收藏
  |  
浏览/下载:16/0
  |  
提交时间:2016/04/12
X-ray binaries
QPO phenomenon
Aquila X-1