Rapid X-ray variability

By M. van der Klis. 2006

319 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/2308b0c0e27c2540370005858fce5e00e9653f50

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Citations in the corpus

Jets from black hole X-ray binaries: testing, refining and extending empirical models for the coupling to X-rays (2009, methodology): “…view of X-ray binary states and state transitions is provided by studying the X-ray variability of such sources, typically on timescales of mHz to kHz, via Fourier power spectra (for recent reviews see van der Klis 2006; Remillard & McClintock 2006; Klein-Wolt & van der Klis 2007; Belloni 2009).”
A global spectral study of black hole X-ray binaries (2009, methodology): “The changes in short timescale timing behaviour e.g. the level of the total rms noise, and the frequency of any quasi-periodical oscillations (QPOs) are frequently used to determine an accurate trnsition date between states (van der Klis 2006).”
Radiatively efficient accreting black holes in the hard state: the case study of H1743-322 (2011, background): “The X-ray transient H1743−322 was discovered with the Ariel V and HEAO I satellites by Kaluzienski & Holt (1977) during a bright outburst in 1977.”
Detecting gravitational wave emission from the known accreting neutron stars (2008, methodology): “The discoveries and studies with the Rossi X-ray Timing Explorer (RXTE) over the last ten years have dramatically improved our understanding of stellar spin rate, νs (Strohmayer & Bildsten 2006; van der Klis 2006).”
Multi-resonance orbital model of high-frequency quasi-periodic oscillations: possible high-precision determination of black hole and neutron star spin (2013, background): “…been observed at low-(Hz) and high-(kHz) frequencies in many Galactic low mass X-ray binaries (LMXBs) containing neutron stars (see, e.g., van der Klis 2000, 2006; Barret et al. 2005b; Belloni et al. 2005, 2007b; Wang et al. 2013)or black holes (see, e.g., McClintock & Remillard 2004; Remillard…”
Relativistic X-Ray Lines from the Inner Accretion Disks Around Black Holes (2007, background): “Quasi-periodic oscillations (QPOs) are common features in the power spectra of accreting stellar-mass black holes and neutron stars (for a review, see van der Klis 2006).”
States and transitions in black-hole binaries (2009, background): “Many neutron-star low-mass X-ray binaries display a transient nature similar to that of black-hole systems (see [95]).”
WATCHDOG: A COMPREHENSIVE ALL-SKY DATABASE OF GALACTIC BLACK HOLE X-RAY BINARIES (2015, background): “In addition, as most BH systems also exhibit rapid temporal variability (e.g., see van der Klis 2006), the observation of low-frequency quasi-periodic oscillations (LFQPOs) can also be used in tandem with spectral characteristics to argue for the presence of a BH (McClintock & Remillard 2006).”
High-frequency quasi-periodic oscillations in black hole binaries (2012, background): “In particular, it is important to compare quantitatively the existing results with those from kilohertz QPOs from neutron star X-ray binaries, where signals are stronger and the known phenomenology much better covered (see e.g. van der Klis 2006 for a review).”
Be/X-ray binaries (2011, background): “3.3 Aperiodic variability Aperiodic variability refers to the variability caused by processes that do not repeat themselves in a periodic way (van der Klis 1995, 2006).”
Formation of millisecond pulsars with CO white dwarf companions – II. Accretion, spin-up, true ages and comparison to MSPs with He white dwarf companions (2012, background): “Although this standard for- c© 0000 RAS mation scenario is commonly accepted many aspects of the mass-transfer process and the accretion physics are still not understood in detail (Lewin & van der Klis 2006).”
The Masses and Spins of Neutron Stars and Stellar-Mass Black Holes (2014, background): “ery stellar-mass black hole shows continuum emission from the disk, as well as disk reﬂection, only a minority show high frequency QPOs, and a smaller minority manifest QPOs in a 3:2 frequency ratio ([292, 312]; note that GRS 1915+105 has two such pairs, one pair at 67 Hz and 41 Hz and the other at ”
TESTING THE NO-HAIR THEOREM WITH EVENT HORIZON TELESCOPE OBSERVATIONS OF SAGITTARIUS A* (2013, background): “Stellar mass black holes are one of the presumed engines that power gamma-ray bursts (Mészáros 2006) and lie at the hearts of X-ray binaries (van der Klis 2006).”