Search Results - "Veledina, Alexandra"
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Interplay of spectral components in timing properties of accreting compact objects
Published in Monthly notices of the Royal Astronomical Society (01-12-2018)“…X-ray variability of accreting black hole binaries is believed to be produced by the fluctuations propagating towards the compact object. Observations suggest…”
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INTERFERENCE AS AN ORIGIN OF THE PEAKED NOISE IN ACCRETING X-RAY BINARIES
Published in The Astrophysical journal (01-12-2016)“…ABSTRACT We propose a physical model for the peaked noise in the X-ray power density spectra of accreting X-ray binaries. We interpret its appearance as an…”
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Accretion geometry of the black hole binary MAXI J1820+070 probed by frequency-resolved spectroscopy
Published in Monthly notices of the Royal Astronomical Society (01-10-2021)“…ABSTRACT The geometry of the inner accretion flow in the hard and hard-intermediate states of X-ray binaries remains controversial. Using Neutron star Interior…”
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Polarized X-Rays from Windy Accretion in Cygnus X-1
Published in Astrophysical journal. Letters (01-05-2023)“…Abstract Recent X-ray polarimetric data on the prototypical black hole X-ray binary Cyg X-1 from the Imaging X-ray Polarimetry Explorer present tight…”
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Hot accretion flow in black hole binaries: a link connecting X-rays to the infrared
Published in Monthly notices of the Royal Astronomical Society (21-04-2013)“…Multiwavelength observations of Galactic black hole transients have opened a new path to understanding the physics of the innermost parts of the accretion…”
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Relativistic Collisionless Shocks in Inhomogeneous Magnetized Plasmas
Published in Astrophysical journal. Letters (01-04-2023)“…Abstract Relativistic collisionless shocks are associated with efficient particle acceleration when propagating into weakly magnetized homogeneous media; as…”
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A UNIFIED LENSE-THIRRING PRECESSION MODEL FOR OPTICAL AND X-RAY QUASI-PERIODIC OSCILLATIONS IN BLACK HOLE BINARIES
Published in The Astrophysical journal (01-12-2013)“…Recent observations of accreting black holes reveal the presence of quasi-periodic oscillations (QPO) in the optical power density spectra. The corresponding…”
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Shock Corrugation to the Rescue of the Internal Shock Model in Microquasars: The Single-scale Magnetohydrodynamic View
Published in The Astrophysical journal (01-04-2023)“…Abstract Questions regarding the energy dissipation in astrophysical jets remain open to date, despite numerous attempts to limit the diversity of the models…”
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Black hole spin-orbit misalignment in the x-ray binary MAXI J1820+070
Published in Science (American Association for the Advancement of Science) (25-02-2022)“…The observational signatures of black holes in x-ray binary systems depend on their masses, spins, accretion rate, and the misalignment angle between the black…”
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A self-consistent hybrid Comptonization model for broad-band spectra of accreting supermassive black holes
Published in Monthly notices of the Royal Astronomical Society (11-07-2011)“…The nature of the broad-band spectra of supermassive accreting black holes in active galactic nuclei (AGNs) is still unknown. The hard X-ray spectra of…”
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Evidence for a Black Hole Spin–Orbit Misalignment in the X-Ray Binary Cyg X-1
Published in Astrophysical journal. Letters (01-07-2023)“…Abstract Recently, the accretion geometry of the black hole X-ray binary Cyg X-1 was probed with the X-ray polarization. The position angle of the…”
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Discovery of correlated optical/X-ray quasi-periodic oscillations in black hole binary SWIFT J1753.5–0127
Published in Monthly notices of the Royal Astronomical Society (11-12-2015)“…We report the discovery of the correlated optical/X-ray low-frequency quasi-periodic oscillations (QPOs) in black hole binary SWIFT J1753.5–0127. The phase lag…”
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Expanding hot flow in the black hole binary SWIFT J1753.5−0127: evidence from optical timing
Published in Monthly notices of the Royal Astronomical Society (01-09-2017)“…Abstract We describe the evolution of optical and X-ray temporal characteristics during the outburst decline of the black hole X-ray binary SWIFT J1753.5−0127…”
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Dramatic Drop in the X-Ray Polarization of Swift J1727.8–1613 in the Soft Spectral State
Published in Astrophysical journal. Letters (01-05-2024)“…Abstract Black hole X-ray binaries exhibit different spectral and timing properties in different accretion states. The X-ray outburst of a recently discovered…”
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Spectroscopic evidence for a low-mass black hole in SWIFT J1753.5−0127
Published in Monthly notices of the Royal Astronomical Society (11-12-2014)Get full text
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Modelling Spectral and Timing Properties of Accreting Black Holes: The Hybrid Hot Flow Paradigm
Published in Space science reviews (01-09-2014)“…The general picture that emerged by the end of 1990s from a large set of optical and X-ray, spectral and timing data was that the X-rays are produced in the…”
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Reprocessing model for the optical quasi-periodic oscillations in black hole binaries
Published in Monthly notices of the Royal Astronomical Society (21-03-2015)“…A number of black hole X-ray transients show quasi-periodic oscillations (QPOs) in the optical (ultraviolet) and X-ray bands at the same frequency, which…”
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Pulsar Wind-heated Accretion Disk and the Origin of Modes in Transitional Millisecond Pulsar PSR J1023+0038
Published in The Astrophysical journal (20-10-2019)“…Transitional millisecond pulsars provide a unique set of observational data for understanding accretion at low rates onto magnetized neutron stars. In…”
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Superhump period of the black hole X-ray binary GX 339−4
Published in Monthly notices of the Royal Astronomical Society (21-08-2018)“…ABSTRACT We investigate the variability of optical and near-infrared light curves of the X-ray binary GX 339−4 on a time-scale of days. We use the data in four…”
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Polarized x-rays constrain the disk-jet geometry in the black hole x-ray binary Cygnus X-1
Published in Science (American Association for the Advancement of Science) (11-11-2022)“…A black hole x-ray binary (XRB) system forms when gas is stripped from a normal star and accretes onto a black hole, which heats the gas sufficiently to emit…”
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