Access the full text.
Sign up today, get DeepDyve free for 14 days.
S. Miyamoto, S. Kitamoto, S. Iga, H. Negoro, K. Terada (1992)
Canonical Time Variations of X-Rays from Black Hole Candidates in the Low-Intensity StateThe Astrophysical Journal, 391
J. Papaloizou, J. Pringle (1984)
The dynamical stability of differentially rotating discs with constant specific angular momentumMonthly Notices of the Royal Astronomical Society, 208
M. Pessah (2009)
ANGULAR MOMENTUM TRANSPORT IN PROTOPLANETARY AND BLACK HOLE ACCRETION DISKS: THE ROLE OF PARASITIC MODES IN THE SATURATION OF MHD TURBULENCEThe Astrophysical Journal, 716
C. Bradshaw, B. Geldzahler, E. Fomalont (2003)
The X-Ray Spectral Changes of Scorpius X-1The Astrophysical Journal, 592
O. Adegoke, S. Rakshit, B. Mukhopadhyay (2016)
Spectral and time series analyses of the Seyfert 1 AGN: Zw 229.015Monthly Notices of the Royal Astronomical Society, 466
S. Rajesh, B. Mukhopadhyay (2009)
Two‐temperature accretion around rotating black holes: a description of the general advective flow paradigm in the presence of various cooling processes to explain low to high luminous sourcesMonthly Notices of the Royal Astronomical Society, 402
P. Grassberger, I. Procaccia (1983)
Measuring the Strangeness of Strange AttractorsPhysica D: Nonlinear Phenomena, 9
M. Klein-Wolt, R. Fender, G. Pooley, T. Belloni, Simone Migliari, E. Morgan, M. Klis (2001)
Hard X‐ray states and radio emission in GRS 1915+105Monthly Notices of the Royal Astronomical Society, 331
(2003)
Does GRS 1915+105 exhibit ``canonical'' black-hole states?
R. Narayan, I. Yi (1994)
Advection dominated accretion: Underfed black holes and neutron starsThe Astrophysical Journal, 452
E. Kuulkers, M. Klis, T. Oosterbroek, J. Paradijs, J. Paradijs, Walter Lewin (1997)
GX 17+2 : X-RAY SPECTRAL AND TIMING BEHAVIOUR OF A BURSTING Z SOURCEMonthly Notices of the Royal Astronomical Society, 287
X. Guan, C. Gammie, J. Simon, B. Johnson (2009)
LOCALITY OF MHD TURBULENCE IN ISOTHERMAL DISKSThe Astrophysical Journal, 694
S. Noble, J. Krolik, J. Hawley (2010)
DEPENDENCE OF INNER ACCRETION DISK STRESS ON PARAMETERS: THE SCHWARZSCHILD CASEThe Astrophysical Journal, 711
J. Lasota (1988)
Slim Accretion DisksThe Astrophysical Journal, 332
T. Belloni, Mariano Méndez, Mariano Méndez, Andrew King, M. Klis, J. Paradijs, J. Paradijs (1997)
A Unified Model for the Spectral Variability in GRS 1915+105The Astrophysical Journal Letters, 488
Yasuo Tanaka, N. Shibazaki (1996)
X-ray novaeAnnual Review of Astronomy and Astrophysics, 34
A. Zdziarski, M. Gierliński (2004)
Radiative Processes, Spectral States and Variability of Black-Hole Binaries(Session 4 : Theoretical/Numerial Approaches to the Accretion Physics)Progress of Theoretical Physics Supplement
M. Kalamkar, M. Reynolds, M. Klis, D. Altamirano, J. Miller (2015)
ARE SPECTRAL AND TIMING CORRELATIONS SIMILAR IN DIFFERENT SPECTRAL STATES IN BLACK HOLE X-RAY BINARIES?The Astrophysical Journal, 802
R. Misra, K. Harikrishnan, Banibrata Mukhopadhyay, G. Ambika, A. Kembhavi (2004)
The Chaotic Behavior of the Black Hole System GRS 1915+105The Astrophysical Journal, 609
L. Burderi, L. Antonelli, F. D’Antona, T. Salvo, G. Israel, L. Piersanti, A. Tornambe', O. Straniero (2005)
Interacting Binaries: Accretion, Evolution, Outcomes, 797
J. Homan, T. Belloni (2004)
The Evolution of Black Hole StatesAstrophysics and Space Science, 300
M. Flock, N. Dzyurkevich, H. Klahr, A. Mignone (2009)
High-order Godunov schemes for global 3D MHD simulations of accretion disks. I. Testing the linear growth of the magneto-rotational instabilityAstronomy and Astrophysics, 516
E. Liang (1998)
MULTI-WAVELENGTH SIGNATURES OF GALACTIC BLACK HOLES : OBSERVATION AND THEORYPhysics Reports, 302
G. Pooley, R. Fender (1997)
The variable radio emission from GRS 1915 + 105Monthly Notices of the Royal Astronomical Society, 292
A. Mignone, G. Bodo, S. Massaglia, T. Matsakos, O. Tesileanu, C. Zanni, A. Ferrari (2007)
PLUTO: A Numerical Code for Computational AstrophysicsThe Astrophysical Journal Supplement Series, 170
U. Das, P. Sharma (2013)
Radiatively inefficient accretion flow simulations with cooling: implications for black hole transientsMonthly Notices of the Royal Astronomical Society, 435
K. Sorathia, C. Reynolds, J. Stone, K. Beckwith (2011)
GLOBAL SIMULATIONS OF ACCRETION DISKS. I. CONVERGENCE AND COMPARISONS WITH LOCAL MODELSThe Astrophysical Journal, 749
S. Chakrabarti, L. Titarchuk (1995)
Spectral Properties of Accretion Disks Around Galactic and Extragalactic Black HolesarXiv: Astrophysics
S. Migliari, T. Belloni (2003)
Evidence for local mass accretion rate variations in the disc of GRS 1915+105Astronomy and Astrophysics, 404
W. Lewin, J. Paradijs, E. Heuvel (2006)
X-ray binaries., 26
J. Hawley, X. Guan, J. Krolik (2011)
ASSESSING QUANTITATIVE RESULTS IN ACCRETION SIMULATIONS: FROM LOCAL TO GLOBALThe Astrophysical Journal, 738
R. Fender, T. Belloni (2004)
GRS 1915+105 and the Disc-Jet Coupling in Accreting Black Hole SystemsAnnual Review of Astronomy and Astrophysics, 42
K. Harikrishnan, R. Misra, G. Ambika, R. Amritkar (2009)
Computing the multifractal spectrum from time series: an algorithmic approach.Chaos, 19 4
D. Leahy, S. Morsink, Y. Chou (2011)
CONSTRAINTS ON THE MASS AND RADIUS OF THE NEUTRON STAR XTE J1807-294The Astrophysical Journal, 742
M. Muno, R. Remillard, D. Chakrabarty (2001)
How Do Z and Atoll X-Ray Binaries Differ?The Astrophysical Journal Letters, 568
R. Remillard, J. McClintock (2006)
X-Ray Properties of Black-Hole BinariesAnnual Review of Astronomy and Astrophysics, 44
H. Tananbaum, H. Gursky, E. Kellogg, R. Giacconi, C. Jones (1972)
Observation of a correlated X-ray-radio transition in Cygnus X-1.The Astrophysical Journal, 177
M. Méndez, V. Klis (1996)
The EXOSAT Data on GX 339–4: Further Evidence for an “Intermediate” StateThe Astrophysical Journal, 479
I. Mirabel, L. Rodríguez, L. Rodríguez (1994)
A superluminal source in the GalaxyNature, 371
Manu Mannattil, H. Gupta, S. Chakraborty (2016)
REVISITING EVIDENCE OF CHAOS IN X-RAY LIGHT CURVES: THE CASE OF GRS 1915+105The Astrophysical Journal, 833
T. Belloni, Diego Altamirano (2006)
High-frequency quasi-periodic oscillations from GRS 1915+105Monthly Notices of the Royal Astronomical Society, 432
B. Karak, Jayanta Dutta, B. Mukhopadhyay (2009)
SEARCH FOR CHAOS IN NEUTRON STAR SYSTEMS: IS Cyg X-3 A BLACK HOLE?The Astrophysical Journal, 708
D. Steeghs, J. Casares (2001)
The Mass Donor of Scorpius X-1 RevealedThe Astrophysical Journal, 568
A. Ingram, C. Done (2011)
A physical model for the continuum variability and QPO in accreting black holesarXiv: Solar and Stellar Astrophysics
T. Gardiner, J. Stone (2005)
An unsplit Godunov method for ideal MHD via constrained transportJournal of Computational Physics, 205
(2004)
PThPS, 155, 99 SOME EXTRA MATERIAL For the spectral fitting of the GRS 1915+105 classes, we consider the energy range 3− 25 keV and the Gaussian line
C. Bradshaw, E. Fomalont, B. Geldzahler (1999)
High-Resolution Parallax Measurements of Scorpius X-1The Astrophysical Journal Letters, 512
M. Abramowicz, Xingming Chen, R. Taam (1995)
The evolution of accretion disks with coronae: A model for the low-frequency quasi-periodic oscillations in X-ray binariesThe Astrophysical Journal, 452
E. Szuszkiewicz, M. Malkan, M. Abramowicz (1995)
The Observational Appearance of Slim Accretion DisksarXiv: Astrophysics
Diego Altamirano, T. Belloni, Manuel Linares, M. Klis, R. Wijnands, P. Curran, M. Kalamkar, H. Stiele, Sara Motta, T. Muñoz-Darias, T. Muñoz-Darias, P. Casella, H. Krimm, H. Krimm (2011)
THE FAINT “HEARTBEATS” OF IGR J17091–3624: AN EXCEPTIONAL BLACK HOLE CANDIDATEThe Astrophysical Journal Letters, 742
R. Misra, K. Harikrishnan, G. Ambika, A. Kembhavi (2006)
The Nonlinear Behavior of the Black Hole System GRS 1915+105The Astrophysical Journal, 643
T. Schreiber, Andreas Schmitz (1996)
Improved Surrogate Data for Nonlinearity Tests.Physical review letters, 77 4
Jochen Greiner, J. Cuby, M. McCaughrean (2001)
An unusually massive stellar black hole in the GalaxyNature, 414
R. Narayan, I. Yi (1994)
Advection-dominated Accretion: A Self-similar SolutionThe Astrophysical Journal, 428
By analysing the time series of RXTE/PCA data, the non-linear variabilities of compact sources have been repeatedly established. Depending on the variation in temporal classes, compact sources exhibit different non-linear features. Sometimes they show low correlation/fractal dimension, but in other classes or intervals of time they exhibit stochastic nature. This could be because the accretion flow around a compact object is a non-linear general relativistic system involving magnetohydrodynamics. However, the more conventional way of addressing a compact source is the analysis of its spectral state. Therefore, the question arises: What is the connection of non-linearity to the underlying spectral properties of the flow when the non-linear properties are related to the associated transport mechanisms describing the geometry of the flow? This work is aimed at addressing this question. Based on the connection between observed spectral and non-linear (time series) properties of two X-ray binaries: GRS 1915+105 and Sco X-1, we attempt to diagnose the underlying accretion modes of the sources in terms of known accretion classes, namely, Keplerian disc, slim disc, advection dominated accretion flow and general advective accretion flow. We explore the possible transition of the sources from one accretion mode to others with time. We further argue that the accretion rate must play an important role in transition between these modes.
Monthly Notices of the Royal Astronomical Society – Oxford University Press
Published: Feb 1, 2018
Keywords: accretion, accretion discs; black hole physics; X-rays: individual: (GRS 1915+105, Sco X−1)
Read and print from thousands of top scholarly journals.
Already have an account? Log in
Bookmark this article. You can see your Bookmarks on your DeepDyve Library.
To save an article, log in first, or sign up for a DeepDyve account if you don’t already have one.
Copy and paste the desired citation format or use the link below to download a file formatted for EndNote
Access the full text.
Sign up today, get DeepDyve free for 14 days.
All DeepDyve websites use cookies to improve your online experience. They were placed on your computer when you launched this website. You can change your cookie settings through your browser.