A shared accretion instability for black holes and neutron stars
暂无分享,去创建一个
K. Long | C. Knigge | N. Degenaar | G. Vasilopoulos | F. Jiménez-Ibarra | J. Neilsen | T. Belloni | D. Altamirano | R. Remillard | S. del Palacio | A. Tetarenko | C. Bailyn | T. Russell | D. Buisson | Y. Cavecchi | M. Armas Padilla | J. van den Eijnden | F. Vincentelli | V. Cúneo | N. Castro Segura | M. Özbey Arabacı | J. Milburn | T. Muñoz Darias | F. Jimenez-Ibarra
[1] A. Ingram,et al. X-ray Eclipse Mapping Constrains the Binary Inclination and Mass Ratio of Swift J1858.6−0814 , 2022, Monthly notices of the Royal Astronomical Society.
[2] J. Bright,et al. Long term radio monitoring of the neutron star X-ray binary Swift J1858.6−0814 , 2022, Monthly notices of the Royal Astronomical Society.
[3] K. Long,et al. A persistent ultraviolet outflow from an accreting neutron star binary transient , 2022, Nature.
[4] Tx,et al. Orbital Decay in M82 X-2 , 2021, The Astrophysical Journal.
[5] C. Knigge,et al. Thermally driven winds in ULXs , 2021, 2110.08249.
[6] D. Walton,et al. Ionised emission and absorption in a large sample of ultraluminous X-ray sources , 2021, Monthly Notices of the Royal Astronomical Society.
[7] D. Walton,et al. Dips and eclipses in the X-ray binary Swift J1858.6–0814 observed with NICER , 2021, Monthly Notices of the Royal Astronomical Society.
[8] D. Walton,et al. Discovery of thermonuclear (Type I) X-ray bursts in the X-ray binary Swift J1858.6–0814 observed with NICER and NuSTAR , 2020, Monthly Notices of the Royal Astronomical Society.
[9] P. Gandhi,et al. Soft X-ray emission lines in the X-ray binary Swift J1858.6–0814 observed with XMM–Newton Reflection Grating Spectrometer: disc atmosphere or wind? , 2020, 2007.14407.
[10] T. Maccarone,et al. The variable radio counterpart of Swift J1858.6-0814 , 2020, Monthly Notices of the Royal Astronomical Society.
[11] R. Salvaterra,et al. The Slow Heartbeats of an Ultraluminous X-Ray Source in NGC 3621 , 2020, The Astrophysical Journal.
[12] J. Tomsick,et al. The obscured X-ray binaries V404 Cyg, Cyg X–3, V4641 Sgr, and GRS 1915+105 , 2020, Astronomy & Astrophysics.
[13] K. Gendreau,et al. The 2019 super-Eddington outburst of RX J0209.6−7427: detection of pulsations and constraints on the magnetic field strength , 2020, Monthly Notices of the Royal Astronomical Society.
[14] C. Knigge,et al. The Changing-look Optical Wind of the Flaring X-Ray Transient Swift J1858.6-0814 , 2020, The Astrophysical Journal.
[15] S. Migliari,et al. Discovery of a thermonuclear Type I X-ray burst in infrared: new limits on the orbital period of 4U 1728-34 , 2020, Monthly Notices of the Royal Astronomical Society: Letters.
[16] Javier A. García,et al. NuSTAR Observations of the Transient Galactic Black Hole Binary Candidate Swift J1858.6–0814: A New Sibling of V404 Cyg and V4641 Sgr? , 2020, The Astrophysical Journal.
[17] S. Tsygankov,et al. Evidence for the radiation-pressure dominated accretion disk in bursting pulsar GRO J1744−28 using timing analysis , 2019, Astronomy & Astrophysics.
[18] K. Gendreau,et al. NGC 300 ULX1: spin evolution, super-Eddington accretion, and outflows , 2019, Monthly Notices of the Royal Astronomical Society.
[19] E. L. Robinson,et al. Optical and X-ray correlations during the 2015 outburst of the black hole V404 Cyg , 2019, Monthly Notices of the Royal Astronomical Society.
[20] R. Fender,et al. A connection between accretion states and the formation of ultrarelativistic outflows in a neutron star X-ray binary , 2018, Monthly Notices of the Royal Astronomical Society.
[21] J. Rodriguez,et al. Optical/X-ray correlations during the V404 Cygni June 2015 outburst , 2018, Astronomy & Astrophysics.
[22] C. Knigge,et al. The evolution of X-ray bursts in the ‘Bursting Pulsar’ GRO J1744–28 , 2018, Monthly Notices of the Royal Astronomical Society.
[23] T. Maccarone,et al. A Wildly Flickering Jet in the Black Hole X-Ray Binary MAXI J1535–571 , 2018, The Astrophysical Journal.
[24] D. Walton,et al. A Potential Cyclotron Resonant Scattering Feature in the Ultraluminous X-Ray Source Pulsar NGC 300 ULX1 Seen by NuSTAR and XMM-Newton , 2018, 1803.07571.
[25] J. G. Bennett,et al. A precise measurement of the magnetic field in the corona of the black hole binary V404 Cygni , 2017, Science.
[26] E. Rosolowsky,et al. Extreme jet ejections from the black hole X-ray binary V404 Cygni , 2017, 1704.08726.
[27] S. Tsygankov,et al. SMC X-3: the closest ultraluminous X-ray source powered by a neutron star with non-dipole magnetic field , 2017, 1702.00966.
[28] V. S. Dhillon,et al. Furiously fast and red: sub-second optical flaring in V404 Cyg during the 2015 outburst peak , 2016, 1603.04461.
[29] Michael Shao,et al. CHIMERA: a wide-field, multi-colour, high-speed photometer at the prime focus of the Hale telescope , 2016, 1601.03104.
[30] Yuki Sugiura,et al. Repetitive patterns in rapid optical variations in the nearby black-hole binary V404 Cygni , 2016, Nature.
[31] J. Zand,et al. Discovery of GRS 1915+105 variability patterns in the Rapid Burster , 2015, 1503.04751.
[32] Agnieszka Janiuk,et al. Interplay between heartbeat oscillations and wind outflow in microquasar IGR J17091-3624 , 2014, 1411.4434.
[33] T. Belloni,et al. Black hole-like hysteresis and accretion states in neutron star low-mass X-ray binaries , 2014, 1407.1318.
[34] Daniel Foreman-Mackey,et al. emcee: The MCMC Hammer , 2012, 1202.3665.
[35] Pas,et al. On different types of instabilities in black hole accretion discs. Implications for X-ray binaries and AGN , 2011, 1102.3257.
[36] P. Reig. Be/X-ray binaries , 2011, 1101.5036.
[37] M. Durant,et al. Rapid optical and X-ray timing observations of GX 339-4: multi-component optical variability in the low/hard state , 2010, 1005.4685.
[38] B. Scott Gaudi,et al. Achieving Better Than 1 Minute Accuracy in the Heliocentric and Barycentric Julian Dates , 2010, 1005.4415.
[39] Philip Kaaret,et al. Ultraluminous X-Ray Sources , 2017, 1703.10728.
[40] N. Gehrels,et al. Rossi X-Ray Timing Explorer Observations of the First Transient Z Source XTE J1701–462: Shedding New Light on Mass Accretion in Luminous Neutron Star X-Ray Binaries , 2006, astro-ph/0610803.
[41] Juri Poutanen,et al. Supercritically accreting stellar mass black holes as ultraluminous X-ray sources , 2006, astro-ph/0609274.
[42] M. Gierliński,et al. Analysing the atolls: X-ray spectral transitions of accreting neutron stars , 2006, astro-ph/0603126.
[43] S. Eikenberry,et al. Observations of Rapid Disk-Jet Interaction in the Microquasar GRS 1915+105 , 2005, astro-ph/0501624.
[44] A. Janiuk,et al. Time‐delays between the soft and hard X‐ray bands in GRS 1915 + 105 , 2004, astro-ph/0409671.
[45] S. Kiyota,et al. Optical Observation of the 2003 Outburst of a Black Hole X-Ray Binary, V4641 Sagittarii , 2004 .
[46] M. Gierliński,et al. GRS 1915+105: the brightest Galactic black hole , 2003, astro-ph/0308536.
[47] A. Moretti,et al. The Quiescent X-Ray Emission of Three Transient X-Ray Pulsars , 2002, astro-ph/0207422.
[48] M. Still,et al. Echoes in X‐ray binaries , 2002, astro-ph/0204018.
[49] I. Kreykenbohm,et al. Magnetic Fields of Accreting X-Ray Pulsars with the Rossi X-Ray Timing Explorer , 2001, astro-ph/0207325.
[50] S. Beard,et al. Ultracam - An Ultra-Fast Triple-Beam CCD Camera , 2001, 0704.2557.
[51] Sera Markoff,et al. A jet model for the broadband spectrum of XTE J1118+480. Synchrotron emission from radio to X-rays in the , 2000, astro-ph/0010560.
[52] A. Janiuk,et al. Radiation Pressure Instability as a Variability Mechanism in the Microquasar GRS 1915+105 , 2000, astro-ph/0008354.
[53] S. Nayakshin,et al. Time-dependent Disk Models for the Microquasar GRS 1915+105 , 1999, astro-ph/9905371.
[54] G. Pooley,et al. Infrared synchrotron oscillations in GRS 1915+105 , 1998, astro-ph/9806073.
[55] R. W. Nelson,et al. Evidence for a Disk-Jet Interaction in the Microquasar GRS 1915+105 , 1997, astro-ph/9710374.
[56] J. Paradijs,et al. A Unified Model for the Spectral Variability in GRS 1915+105 , 1997, astro-ph/9708113.
[57] W. Paciesas,et al. Hard X-Ray Signature of Plasma Ejection in the Galactic Jet Source GRS 1915+105 , 1997 .
[58] A. R. King,et al. An Unstable Central Disk in the Superluminal Black Hole X-Ray Binary GRS 1915+105 , 1997, astro-ph/9702048.
[59] P. M. Williams,et al. Flaring and quiescent infrared behaviour of Cygnus X-3 , 1996 .
[60] R Edelson,et al. The Discrete Correlation Function: a New Method for Analyzing Unevenly Sampled Variability Data , 1988 .
[61] Roger D. Blandford,et al. Particle acceleration at astrophysical shocks: A theory of cosmic ray origin , 1987 .
[62] A. Bell. The acceleration of cosmic rays in shock fronts – I , 1978 .
[63] Douglas M. Eardley,et al. Black Holes in Binary Systems: Instability of Disk Accretion , 1974 .
[64] H. Laan,et al. A Model for Variable Extragalactic Radio Sources , 1966, Nature.