Insight-HXMT observations of jet-like corona in a black hole X-ray binary MAXI J1820+070

Hongwei Liu | Xinying Song | Bing Li | Zhao Zhang | Yi Zhang | Z. Dai | W. Cui | Gang Chen | M. Gao | C. Luo | Yinong Liu | S. Xiong | X. Wen | Yanguo Li | Xiaohua Liang | Xiaojing Liu | Sheng Yang | Fan. Zhang | C. Cai | S. Xiao | Q. Yi | Qingwen Wu | He Gao | C. Jin | Shuang-Nan Zhang | R. Shang | F. Lu | T. Luo | Tipei Li | Jifeng Liu | Zhu Liu | Chen Wang | G. Xiao | L. Tao | Yong Chen | B. Czerny | Tianxiang Chen | Yupeng Xu | Shu Zhang | Xuefeng Lu | Yuxuan Zhu | Yusa Wang | Xiaobo Li | Xufang Li | Y. Tan | Yanji Yang | M. Ge | Juan Zhang | B. Wu | J. Liao | Yifei Zhang | Liming Song | Congzhan Liu | Jianyin Nie | Haisheng Zhao | Chengkui Li | Xiaofa Zhao | W. Yuan | Lingjun Wang | Yongjie Jin | A. Zhang | Bobing Wu | Mei Wu | Yongjie Zhang | J. Huo | Juan Wang | Wei Li | Yue Zhu | Q. Luo | Z. Chang | Y. Tuo | Q. Bu | M. Fu | G. Gao | J. Guan | S. Jia | L. Kong | B. Meng | Y. Nang | G. Ou | N. Sai | Q. Yin | Y. You | Chengzhe Li | Gang Li | Yue Huang | Zhengwei Li | Chengmo Zhang | Jia-wei Yang | Liang Sun | Luhua Jiang | B. Lu | B. You | Ziliang Zhang | Dawei Han | Maoshun Li | Bi-fang Liu | Yue Zhang | Xian Li | D. Zhou | E. Qiao | Jing-kang Deng | Wenzhao Zhang | Xiang Ma | Wei Zhang | Shijie Zheng | Li Chen | Guofeng Wang | Tong Zhang | Guoqing Liu | H. Gao | Wenshuai Wang | Yudong Gu | J. Jin | Cheng-Cheng Guo | X. Cao | W. Jiang | Wanchang Zhang | Y. Du | Wen Wang | Hongmei Zhang | Y. Dong | Yu-Peng Chen | Yibao Chen | Jinlu Qu | Jian-feng Zhou | Yongwei Dong | Jinyuan Liao | Weichun Jiang | X. Ma | Qingwen Wu | Xiang Ma | Xue-Feng Lu | Baiyang Wu | Bifang Liu

[1]  Wei Zhang,et al.  Discovery of oscillations above 200 keV in a black hole X-ray binary with Insight-HXMT , 2020, Nature Astronomy.

[2]  F. Harrison,et al.  NuSTAR low energy effective area correction due to thermal blanket tear , 2020, 2005.00569.

[3]  Y. N. Liu,et al.  The Evolution of the Broadband Temporal Features Observed in the Black-hole Transient MAXI J1820+070 with Insight-HXMT , 2020, The Astrophysical Journal.

[4]  D. Walton,et al.  The soft state of the black hole transient source MAXI J1820+070: emission from the edge of the plunge region? , 2020, Monthly Notices of the Royal Astronomical Society.

[5]  Zhen Yan,et al.  Coronal Properties of Black Hole X-Ray Binaries in the Hard State as Seen by NuSTAR and Swift , 2019, The Astrophysical Journal.

[6]  A. Deller,et al.  A radio parallax to the black hole X-ray binary MAXI J1820+070 , 2019, Monthly Notices of the Royal Astronomical Society: Letters.

[7]  D. Walton,et al.  MAXI J1820+070 with NuSTAR I. An increase in variability frequency but a stable reflection spectrum: coronal properties and implications for the inner disc in black hole binaries , 2019, Monthly Notices of the Royal Astronomical Society.

[8]  Qingwen Wu,et al.  Evolution of the hard X-ray photon index in black-hole X-ray binaries: hints for accretion physics , 2019, Monthly Notices of the Royal Astronomical Society.

[9]  P. Jonker,et al.  Dynamical Confirmation of a Black Hole in MAXI J1820+070 , 2019, The Astrophysical Journal.

[10]  N. Kawai,et al.  X-Ray and Optical Monitoring of State Transitions in MAXI J1820+070 , 2019, The Astrophysical Journal.

[11]  P. Uttley,et al.  The corona contracts in a black-hole transient , 2019, Nature.

[12]  N. Kawai,et al.  X-Ray, Optical, and Near-infrared Monitoring of the New X-Ray Transient MAXI J1820+070 in the Low/Hard State , 2018, The Astrophysical Journal.

[13]  L. M. Song,et al.  Insight-HXMT science operations , 2018, Astronomical Telescopes + Instrumentation.

[14]  S. Eikenberry,et al.  NICER observations of MAXI J1820+070 : Continuing evolution of X-ray variability properties , 2018 .

[15]  Xiaofeng Wang,et al.  Detection of optical and X-ray QPOs at similar frequencies in MAXI J1820+070 , 2018 .

[16]  D. J. Walton,et al.  Exponential increase in X-ray QPO frequency with time in MAXI J1820+070 , 2018 .

[17]  S. Trushkin,et al.  The 30-day monitoring of MAXI J1820+070 at 4.7 GHz , 2018 .

[18]  P. Bult,et al.  NICER observations of MAXI J1820+070 suggest a rapidly-brightening black hole X-ray binary in the hard state , 2018 .

[19]  C. Littlefield Fast optical flaring in the suspected black-hole binary MAXI J1820+070 (ASASSN-18ey) , 2018 .

[20]  S. Littlefair,et al.  Red sub-second optical flaring in MAXI J1820+070 observed by ULTRACAM/NTT , 2018 .

[21]  Naoki Isobe,et al.  MAXI/GSC detection of a probable new X-ray transient MAXI J1820+070 , 2018 .

[22]  D. Palmer,et al.  Swift detection of MAXI J1820+070 , 2018 .

[23]  P. Garnavich,et al.  Optical Spectra of MAXI J1820+070 with Keck , 2018 .

[24]  R. Burenin,et al.  Low-frequency QPOs in MAXI J1820+070 as seen by INTEGRAL/SPI , 2018 .

[25]  J. Strader,et al.  SOAR/Goodman optical spectroscopy of MAXI J1820+070 , 2018 .

[26]  Masaomi Tanaka,et al.  Detection of 10-msec scale optical flares in the black-hole binary candidate MAXI J1820+070 (ASASSN-18ey) , 2018 .

[27]  Fraser Lewis,et al.  Optical observations of MAXI J1820+070 suggest it is a black hole X-ray binary , 2018 .

[28]  Javier A. García,et al.  Alternative Explanations for Extreme Supersolar Iron Abundances Inferred from the Energy Spectrum of Cygnus X-1 , 2018, 1801.07267.

[29]  Javier A. García,et al.  The effects of high density on the X-ray spectrum reflected from accretion discs around black holes , 2016, 1603.05259.

[30]  D. Walton,et al.  Normalizing a Relativistic Model of X-ray Reflection: The Definition of the Reflection Fraction and its Implementation in relxill , 2016, 1601.03771.

[31]  D. Walton,et al.  THE COMPLEX ACCRETION GEOMETRY OF GX 339–4 AS SEEN BY NuSTAR AND SWIFT , 2015, 1506.01381.

[32]  D. Walton,et al.  NuSTAR AND SUZAKU OBSERVATIONS OF THE HARD STATE IN CYGNUS X-1: LOCATING THE INNER ACCRETION DISK , 2015, 1506.00007.

[33]  F. J. Lu,et al.  Introduction to the hard x-ray modulation telescope , 2014, Astronomical Telescopes and Instrumentation.

[34]  G. Ponti,et al.  Revealing accretion on to black holes: X-ray reflection throughout three outbursts of GX 339−4 , 2014, 1404.7498.

[35]  R. Narayan,et al.  Hot Accretion Flows Around Black Holes , 2014, 1401.0586.

[36]  T. Dauser,et al.  X-RAY REFLECTED SPECTRA FROM ACCRETION DISK MODELS. III. A COMPLETE GRID OF IONIZED REFLECTION CALCULATIONS , 2013, 1303.2112.

[37]  Daniel Foreman-Mackey,et al.  emcee: The MCMC Hammer , 2012, 1202.3665.

[38]  A. Fabian,et al.  Understanding X‐ray reflection emissivity profiles in AGN: locating the X‐ray source , 2012, 1205.3179.

[39]  B. Liu,et al.  THE EMISSION FROM AN INNER DISK AND A CORONA IN THE LOW AND INTERMEDIATE SPECTRAL STATES OF BLACK HOLE X-RAY BINARIES , 2011, 1109.5824.

[40]  A. Fabian,et al.  Determination of the X-ray reflection emissivity profile of 1H 0707-495 , 2011, 1102.0433.

[41]  J. García,et al.  X-RAY REFLECTED SPECTRA FROM ACCRETION DISK MODELS. II. DIAGNOSTIC TOOLS FOR X-RAY OBSERVATIONS , 2011, 1101.1115.

[42]  Naoki Isobe,et al.  The MAXI Mission on the ISS: Science and Instruments for Monitoring All-Sky X-Ray Images , 2009, 0906.0631.

[43]  Xinwu Cao An accretion disc-corona model for X-ray spectra of active galactic nuclei , 2008, 0812.1828.

[44]  Aya Kubota,et al.  Modelling the behaviour of accretion flows in X-ray binaries , 2007, 0708.0148.

[45]  S. Nayakshin,et al.  On the X-ray reflected spectra from accretion disk models , 2005 .

[46]  S. Markoff,et al.  Going with the Flow: Can the Base of Jets Subsume the Role of Compact Accretion Disk Coronae? , 2005, astro-ph/0509028.

[47]  T. Belloni,et al.  GRS 1915+105 and the Disc-Jet Coupling in Accreting Black Hole Systems , 2004, astro-ph/0406483.

[48]  M. Gierliński,et al.  Radiative Processes, Spectral States and Variability of Black-Hole Binaries(Session 4 : Theoretical/Numerial Approaches to the Accretion Physics) , 2004, astro-ph/0403683.

[49]  U. Tokyo,et al.  The Three Spectral Regimes Found in the Stellar Black Hole XTE J1550–564 in Its High/Soft State , 2003, astro-ph/0310085.

[50]  J. Wilms,et al.  Absorption Of X-rays In The Interstellar Medium , 2000, astro-ph/0008425.

[51]  C.S.Reynolds,et al.  Broad iron lines in Active Galactic Nuclei , 2000, astro-ph/0004366.

[52]  Andrew C. Fabian,et al.  Broad Iron Lines in Active Galactic Nuclei , 2000 .

[53]  A. M. Beloborodov Plasma Ejection from Magnetic Flares and the X-Ray Spectrum of Cygnus X-1 , 1999 .

[54]  A. Zdziarski,et al.  Black hole accretion disks with coronae , 1994 .

[55]  Paolo S. Coppi,et al.  Time-dependent models of magnetized pair plasmas , 1992 .

[56]  G. Henri,et al.  Relativistic electron-positron beam formation in the framework of the two-flow model for active galactic nuclei , 1991 .

[57]  K. Koyama,et al.  Energy spectra of low-mass binary X-ray sources observed from TENMA , 1984 .

[58]  F P Retief,et al.  [The first ten years]. , 1979, South African medical journal = Suid-Afrikaanse tydskrif vir geneeskunde.

[59]  Robert E. Wilson,et al.  BLACK HOLES IN BINARY SYSTEMS , 1973 .

[60]  Rashid Sunyaev,et al.  Black holes in binary systems. Observational appearance , 1973 .