机构

• 国家天文台 [5]
• 高能物理研究所 [3]
• 新疆天文台 [3]
• 理论物理研究所 [1]

采集方式

• OAI收割 [12]

内容类型

• 期刊论文 [12]

发表日期

• 2022 [2]
• 2021 [1]
• 2020 [5]
• 2019 [2]
• 2018 [1]
• 2005 [1]
• 更多

学科主题

• Astronomy ... [1]
• Physics [1]
• 星系和宇宙学 [1]

筛选

浏览/检索结果: 共12条，第1-10条 帮助 条数/页： 5101520253035404550556065707580859095100 排序方式： 请选择提交时间升序提交时间降序发表日期升序发表日期降序题名升序题名降序作者升序作者降序 Searching for strange quark matter objects among white dwarfs 期刊论文  OAI收割 PHYSICS LETTERS B, 2022, 卷号: 832, 页码: 6 作者:  Kurban, Abdusattar;  Huang, Yong-Feng;  Geng, Jin-Jun;  Zong, Hong-Shi   |  收藏  |  浏览/下载：22/0  |  提交时间：2023/02/28 Compact objects  Strange quark matter  Strange quark stars   The Wide Field Monitor onboard the Chinese-European X-ray mission eXTP 期刊论文  OAI收割 SPACE TELESCOPES AND INSTRUMENTATION 2022: ULTRAVIOLET TO GAMMA RAY, 2022, 卷号: 12181, 页码: 121811Y 作者:  eXTP   |  收藏  |  浏览/下载：4/0  |  提交时间：2023/11/09 X-ray timing  X-ray spectroscopy  compact objects: black holes  neutron stars and white dwarfs  gamma-ray bursts  X-ray bursts  gravitational wave events  silicon drift detectors  coded mask imaging   Refined Mass and Geometric Measurements of the High-mass PSR J0740+6620 期刊论文  OAI收割 The Astrophysical Journal Letters, 2021, 卷号: 915, 期号: 1 作者:  Fonseca,E.;  Cromartie,H. T.;  Pennucci,T. T.;  Ray,P. S.;  Kirichenko,A. Yu.   |  收藏  |  浏览/下载：13/0  |  提交时间：2021/12/06 Neutron stars  Pulsars  General relativity  Compact objects  Binary pulsars   Formation and Evolution of Ultraluminous X-Ray Pulsar Binaries to Pulsar-Neutron Star and Pulsar-White Dwarf Systems 期刊论文  OAI收割 The Astrophysical Journal, 2020, 卷号: 902, 页码: 125 作者:  Abdusalam, K.;  Ablimit, Iminhaji;  Hashim, P.;  Lü, G. -L.;  Mardini, M. K.   |  收藏  |  浏览/下载：41/0  |  提交时间：2021/06/25 Binary stars  Close binary stars  X-ray binary stars  Pulsars  Gravitational wave sources  White dwarf stars  Compact objects  154  254  1811  1306  677  1799  288  Astrophysics - High Energy  Astrophysical Phenomena   Formation and Evolution of Ultraluminous X-Ray Pulsar Binaries to Pulsar–Neutron Star and Pulsar–White Dwarf Systems 期刊论文  OAI收割 The Astrophysical Journal, 2020, 卷号: 902, 期号: 2 作者:  Abdusalam,K.;  Ablimit,Iminhaji;  Hashim,P.;  Lü,G.-L;  Mardini,M. K.   |  收藏  |  浏览/下载：20/0  |  提交时间：2021/12/06 Binary stars  Close binary stars  X-ray binary stars  Pulsars  Gravitational wave sources  White dwarf stars  Compact objects   Discovery of the Black Hole X-Ray Binary Transient MAXI J1348–630 期刊论文  OAI收割 The Astrophysical Journal Letters, 2020, 卷号: 899, 期号: 1 作者:  Tominaga,Mayu;  Nakahira,Satoshi;  Shidatsu,Megumi;  Oeda,Motoki;  Ebisawa,Ken   |  收藏  |  浏览/下载：11/0  |  提交时间：2021/12/06 Black holes  Compact objects  High energy astrophysics  X-ray novae  Stellar accretion disks   The Evolution of the Broadband Temporal Features Observed in the Black-hole Transient MAXI J1820+070 with Insight-HXMT 期刊论文  OAI收割 The Astrophysical Journal, 2020, 卷号: 896, 期号: 1 作者:  Wang,Yanan;  Ji,Long;  Zhang,S. N.;  Méndez,Mariano;  Qu,J. L.   |  收藏  |  浏览/下载：26/0  |  提交时间：2021/12/06 Black holes  Compact objects  Low-mass x-ray binary stars   Introducing a special collection of papers in the Journal of High Energy Astrophysics on the Early Results of China's 1st X-ray Astronomy Satellite: Insight-HXMT 期刊论文  OAI收割 Journal of High Energy Astrophysics, 2020, 卷号: 27, 页码: 51-52 作者:  HXMT   |  收藏  |  浏览/下载：36/0  |  提交时间：2022/02/08 Astrophysics - High Energy Astrophysical Phenomena  Abstract: Insight-HXMT is the first Chinese X-ray astronomical mission, launched successfully on June 15, 2017, from China's Jiuquan Satellite Launch Center. Insight-HXMT was designed to have a broad energy coverage in X-rays, from 1-250 keV, with excellent timing and adequate energy resolution at soft X-rays, and the largest effective area at hard X-rays. This allows, in particular, to observe bright sources like X-ray binaries (XRBs) in their bright/outburst states with high cadence and high statistics at hard and soft X-rays at once. It was then expected that the Insight-HXMT mission will bring us new insights regarding the characteristics of several source classes. Examples include characterizing High-Mass X-ray Binaries (HMXBs) and the outburst evolution of Low-Mass X-ray Binaries (LMXBs). For instance, in HMXB systems, the region around their Alfven radius that is responsible to determine whether accretion or propeller occurs, or the region around the NS magnetic pole where the intense X-rays are supposed to be produced are specially appealing targets of study. For the LMXBs, the evolution the outburst and the properties of the compact objects themselves are obvious priority targets for Insight-HXMT. Due to the broad coverage in energy, Insight-HXMT is specially well suited to study the influence of thermonuclear (type-I) X-ray bursts upon the surrounding environment.   Populations of Stellar-mass Black Holes from Binary Systems 期刊论文  OAI收割 The Astrophysical Journal, 2019, 卷号: 885, 期号: 1 作者:  Wiktorowicz,Grzegorz;  Wyrzykowski,?ukasz;  Chruslinska,Martyna;  Klencki,Jakub;  Rybicki,Krzysztof A.   |  收藏  |  浏览/下载：5/0  |  提交时间：2020/03/10 Black holes  Astrophysical black holes  Stellar populations  Binary stars  X-ray binary stars  Compact objects  Gravitational microlensing  Gravitational waves  Stellar evolution   Using LISA-like gravitational wave detectors to search for primordial black holes 期刊论文  OAI收割 PHYSICAL REVIEW D, 2019, 卷号: 99, 期号: 2, 页码: 23001 作者:  Guo, HK;  Shu, J;  Zhao, Y   |  收藏  |  浏览/下载：55/0  |  提交时间：2019/07/19 SUPERMASSIVE COMPACT OBJECTS  STRONG MASS SEGREGATION  DARK-MATTER  COSMOLOGICAL ABUNDANCE  FUNDAMENTAL RELATION  LIMITS  RELAXATION  RADIATION