机构

• 新疆天文台 [2]
• 云南天文台 [2]
• 高能物理研究所 [1]

采集方式

• OAI收割 [5]

内容类型

• 期刊论文 [5]

发表日期

• 2021 [5]

学科主题

• 天文学 [2]
• 天文学::天体物理学 [2]
• 天文学::天体物理学... [2]
• 天文学::恒星与银河... [2]
• 天文学::恒星与银河... [2]
• 天文学::天体物理学... [1]
• 更多

筛选

浏览/检索结果: 共5条，第1-5条 帮助 限定条件 发表日期：2021     条数/页： 5101520253035404550556065707580859095100 排序方式： 请选择提交时间升序提交时间降序题名升序题名降序作者升序作者降序发表日期升序发表日期降序 Optical and ultraviolet monitoring of the black hole X-ray binary MAXI J1820+070/ASASSN-18ey for 18 months 期刊论文  OAI收割 MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2021, 卷号: 504, 期号: 3, 页码: 4226-4241 作者:  Sai, Hanna;  Wang, Xiaofeng;  Wu, Jianfeng;  Lin, Jie;  Feng, Hua   |  收藏  |  浏览/下载：36/0  |  提交时间：2021/07/24 accretion, accretion discs  stars: black holes  X-rays: binaries   A study on the hysteresis effect and spectral evolution in the mini-outbursts of balck hole X-ray binary XTE J1550-564 期刊论文  OAI收割 Frontiers in Astronomy and Space Sciences, 2021, 卷号: 8, 页码: 37 作者:  Dong, Ai-Jun;  Liu, Chang;  Ge, Kang;  Liu, Xiang;  Zhi, Qi-Jun   |  收藏  |  浏览/下载：19/0  |  提交时间：2022/06/30 accretion  accretion discs  stars: black holes  X-ray binaries  -X-rays: individual: XTE J1550-564   Possible evidence of a universal radio/X-ray correlation in a near-complete sample of hard X-ray selected seyfert galaxies 期刊论文  OAI收割 MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2021, 卷号: 503, 期号: 2, 页码: 1987-1998 作者:  Chang, N.;  Xie, F. G.;  Liu, X.;  Ho, L. C.;  Dong, A-J   |  收藏  |  浏览/下载：91/0  |  提交时间：2021/11/09 accretion, accretion discs  galaxies: active  galaxies: Seyfert  radio continuum: galaxies   Three-dimensional simulations of accretion flow in the progenitor of Tycho's supernova 期刊论文  OAI收割 MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2021, 卷号: 501, 期号: 1, 页码: 664-675 作者:     |  收藏  |  浏览/下载：12/0  |  提交时间：2021/03/08 accretion, accretion discs  hydrodynamics  methods: numerical  binaries: general  supernovae: individual: SN 1572 (Tycho's supernova)  white dwarfs   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：42/0  |  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.