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Related papers: Boundary layer emission in luminous LMXBs

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We study the kilohertz quasi-periodic oscillations (kHz QPOs) and the band-limited noise (BLN) in the 0.5--16 Hz range observed simultaneously on the horizontal branch (HB) and on the upper normal branch (NB) of the brightest neutron star…

Astrophysics · Physics 2011-02-11 Xiaofeng Cao , Wenfei Yu

X-ray emission from AGN is dominated by the accretion disk around a SMBH. The radio luminosity, however, has not such a clear origin except in the most powerful sources where jets are evident. The origin (and even the very existence) of the…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 L. Ballo , F. J. H. Heras , X. Barcons , F. J. Carrera

The origin of the large-amplitude, quasi-periodic X-ray flux variations in several classes of the Galactic microquasar GRS~1915+105 remains unresolved. We address this issue through flux-resolved, broadband (0.8-20 keV) spectral modelling…

High Energy Astrophysical Phenomena · Physics 2026-02-13 Shree Suman , Shuvajit Khatua , Vishal Jadoliya , Prathamesh Narayan Gupta , Mayukh Pahari

We have investigated the spectral and timing variability of four accreting X-ray pulsars with Be-type companions during major X-ray outbursts. Different spectral states were defined according to the value of the X-ray colours and flux.…

Astrophysics · Physics 2009-11-13 P. Reig

LS 5039 is an X-ray binary that presents non-thermal radio emission. The radiation at $\sim 5$ GHz is quite steady and optically thin, consisting on a dominant core plus an extended jet-like structure. There is a spectral turnover around 1…

Astrophysics · Physics 2009-11-13 V. Bosch-Ramon

In 2021 BL Lacertae underwent an extraordinary activity phase, which was intensively followed by the Whole Earth Blazar Telescope (WEBT) Collaboration. We present the WEBT optical data in the BVRI bands acquired at 36 observatories around…

We develop a model for steady, laminar boundary layers over small-scale textured surfaces. Although the texture is small relative to the boundary-layer thickness, it modifies the flow via a slip length. We use matched asymptotic expansions…

Fluid Dynamics · Physics 2026-02-27 Samuel D. Tomlinson , Demetrios T. Papageorgiou

We have observed S4 0954+658 in the BVRI bands in 2001, and in the BI bands in 2002. The observations resulted in almost evenly sampled light curves, 3-8 hours long, with an average sampling interval of ~5-15 min. Because of the dense…

Astrophysics · Physics 2009-11-10 I. E. Papadakis , V. Samaritakis , P. Boumis , J. Papamastorakis

We study how bulk propagation in global AdS$_3$ is encoded in boundary energy densities of the dual CFT$_2$ on the cylinder. A key feature of the global geometry, which is absent in the Poincar\'e-patch description, is that a null…

High Energy Physics - Theory · Physics 2026-05-29 Shiki Yoshikawa

We report on a detailed analysis of the so-called ~1 Hz quasi-periodic oscillation (QPO) in the eclipsing and dipping neutron-star low-mass X-ray binary EXO 0748-676. This type of QPO has previously been shown to have a geometric origin.…

High Energy Astrophysical Phenomena · Physics 2015-11-13 Jeroen Homan , Joel K. Fridriksson , Ronald A. Remillard

The conventional Ekman model of the tropical boundary layer neglects nonlinear momentum advection and breaks down near the equator, where Coriolis effects are weak. During South Asian monsoon onset, we identify a dynamical regime transition…

Atmospheric and Oceanic Physics · Physics 2026-03-10 Rajat Masiwal , Ashwin K Seshadri , Vishal Dixit

Low Frequency Quasi-Periodic Oscillations or LF QPOs are ubiquitous in BH X-ray binaries and provide strong constraints on the accretion-ejection processes. Although several models have been proposed so far, none has been proven to…

The transient atoll source 4U 1608-52 had been extensively observed by the Rossi X-ray Timing Explorer RXTE during its 1998 outburst. We analyse its X-ray spectra as a function of inferred accretion rate from both the 1998 outburst and from…

Astrophysics · Physics 2009-11-07 Marek Gierlinski , Chris Done

In this letter, we suggest that the missing boundary layer luminosity of dwarf novae in quiescence is released mainly in the ultraviolet (UV) as the second component commonly identified in the far ultraviolet (FUV) as the "accretion belt".…

Astrophysics · Physics 2009-11-10 Patrick Godon , Edward M. Sion

We study the stochastic variation of blazar emission under a 2-D spatially resolved leptonic jet model we previously developed. Random events of particle acceleration and injection in small zones within the emission region are assumed to be…

High Energy Astrophysical Phenomena · Physics 2016-03-23 Xuhui Chen , Martin Pohl , Markus Böttcher , Shan Gao

Blazars show variability on timescales ranging from minutes to years, the former being comparable to and in some cases even shorter than the light-crossing time of the central black hole. The observed gamma-ray lightcurves can be described…

High Energy Astrophysical Phenomena · Physics 2017-07-10 Michael O' Riordan , Asaf Pe'er , Jonathan C. McKinney

Theory and observations of the dominant thermal continuum emission in AGNs are examined. After correction for reddening, the steady state AGN optical--UV spectral energy distributions (SEDs) are very similar. The SEDs are dominated…

Astrophysics · Physics 2007-11-15 C. Martin Gaskell

Boundary conditions may change the phase diagram of non-equilibrium statistical systems like the one-dimensional asymmetric simple exclusion process with and without particle number conservation. Using the quantum Hamiltonian approach, the…

High Energy Physics - Theory · Physics 2009-10-22 Malte Henkel , Gunter Schütz

The BL Lac object Mkn~421 was observed three times by the X-ray observatory BeppoSAX in consecutive days during 1997 April and May. The source was in a quiescent state, with an average 2-10 keV flux of 9.0 x 10^(-11) erg/cm/cm/s. Flux…

Astrophysics · Physics 2007-05-23 M. Guainazzi , G. Vacanti , A. Malizia , K. S. O'Flaherty , E. Palazzi , A. N. Parmar

Exploiting the presence of kilohertz quasi-periodic oscillations (QPOs) in the timing power spectrum, we find that the soft x-ray emission of the neutron-star X-ray binary and atoll source 4U1636-536 modulated at the QPO frequency lags…

Astrophysics · Physics 2009-10-31 Philip Kaaret , Santina Piraino , Eric C. Ford , Andrea Santangelo