Characterizing the Quasi-periodic Oscillation Behavior of the X-Ray Nova XTE J1550–564

By Ronald A. Remillard, G. Sobczak, M. Muno, J. E. McClintock. 2002

144 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Biomedical Engineering, Geophysics

View Paper: https://www.semanticscholar.org/paper/a657de9606cc7041b90db2b6863e52f13ce72a87

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Citations in the corpus

The spin of the black hole microquasar XTE J1550−564 via the continuum-fitting and Fe-line methods (2010, background): “…X-ray spectral and timing properties of this source have been comprehensively studied by many authors (e.g. Sobczak et al. 2000; Homan et al. 2001; Remillard et al. 2002b; Kubota & Done 2004; Dunn et al. 2010), as have been the properties of its radio counterpart (Corbel et al. 2001; Xue, Wu &…”
A Unified Model for Black Hole X-Ray Binary Jets? (2004, background): “The data analysed her correspond to the brightest one, in 1998/1999 (see Sobczak et l. 2000; Homan et al. 2001; Remillard et al. 2002).”
WATCHDOG: A COMPREHENSIVE ALL-SKY DATABASE OF GALACTIC BLACK HOLE X-RAY BINARIES (2015, unknown): “…Mangano et al. (2010a), [136] Kuulkers et al. (2013), [137] Yamaoka et al. (2012), [138] Ferrigno et al. (2011), [139] Negoro et al. (2011b), [140] Remillard et al. (2002), [141] Russell et al. (2014a), [142] in ’t Zand et al. (2001), [143] in’t Zand et al. (2002c), [144] Wijnands & Miller…”
High-frequency quasi-periodic oscillations in black hole binaries (2012, background): “There are 20 detections reported in Remillard et al. (2002a) from the 1998 outburst of XTE J1550-564.”
The Evolution of Black Hole States (2004, background): “Currently three types of these low-frequency QPOs are recognized in black hole binaries, called type A, B and C (Wijnands et al., 1999, Remillard et al., 2002).”
The evolution of the timing properties of the black-hole transient GX 339-4 during its 2002/2003 outburst (2005, unknown): “These phase lags are in marked contrast with what is usually observed in VHS observations, where the type-C QPO shows soft lags (see Wijnands et al. 1999; Reig et al. 2000; Homan et al. 2001; Remillard et al. 2002; Casella et al. 2004).”
Evidence for Harmonic Relationships in the High-Frequency Quasi-periodic Oscillations of XTE J1550–564 and GRO J1655–40 (2002, methodology): “A major outburst during 1998–1999 revealed complex evolution in both its spectral properties and variability characteristics (Wijnands, Homan, & van der Klis 1999; Sobczak et al. 2000b; Homan et al. 2001; Remillard et al. 2002).”
Multiwavelength Observations of the 2002 Outburst of GX 339–4: Two Patterns of X-Ray-Optical/Near-Infrared Behavior (2005, background): “Note that during the intermediate state, on MJD 52,402, the disk flux showed a dramatic increase without substantially changing or interrupting the evolution of the power-law index and type C QPO frequencies (seeWijnands et al. 1999 and Remillard et al. 2002 for a definition of QPO types).”
The Three Spectral Regimes Found in the Stellar Black Hole XTE J1550–564 in Its High/Soft State (2003, unknown): “Interestingly, the quasi-periodic oscillations (QPOs) are observed preferentially in the anomalous regime, in GRO J1655 − 40 (Remillard et al. 1999) and XTE J1550 − 564 (Remillard et al. 2002).”
X-Ray Properties of Black-Hole Binaries (2006, methodology): “The four sources that exhibit harmonic pairs of frequencies in a 3:2 ratio (see §6.2) suggest that HFQPOs arise from some type of resonance mechanism (Abramowicz & Kluźniak 2001; Remillard et al. 2002a).”
The ABC of Low-Frequency Quasi-periodic Oscillations in Black Hole Candidates: Analogies with Z Sources (2005, background): “…trend towards soft lags (i.e. soft X-ray variations lag those at hard X-ray energies) for increasing QPO frequency (see Reig et al. 2000), but they are usually consistently soft at the subharmonic and hard at the second harmonic (see e.g. Remillard et al. 2002; Casella et al. 2004, C04 hereafter).”
AN IMPROVED DYNAMICAL MODEL FOR THE MICROQUASAR XTE J1550−564 (2011, background): “It is one of seven sources of high-frequency quasi-periodic oscillations (QPOs), and it is only one of four such sources that exhibit harmonic pairs of frequencies in a 3:2 ratio (Miller et al. 2001; Remillard et al. 2002a; Remillard & McClintock 2006).”
A study of the low-frequency quasi-periodic oscillations in the X-ray light curves of the black hole candidate XTE J1859+226 (2004, methodology): “Observations with the Rossi X-ray Timing Explorer (RXTE) have led to an extraordinary progress in the knowledge of the variability properties of black-hole candidates (BHCs) in X-ray binaries (see e.g. van der Klis 2000 and Remillard et al. 2002a).”
A physical model for the continuum variability and QPO in accreting black holes (2011, methodology): “We fit this model to a sequence of power spectra of XTE J1550-564 observed during a transition from low/hard to intermediatestate, and show that these give a goodquantitativefit for ro moving from ∼ 75 − 10Rg , as also required to explain the sequence in energy spectra during this transition.”