Boundary layer emission in luminous LMXBs
arXiv:astro-ph/0512361 · doi:10.1002/asna.200510419
Abstract
We show that aperiodic and quasiperiodic variability of bright LMXBs - atoll and Z- sources, on ~sec - msec time scales is caused primarily by variations of the boundary layer luminosity. The accretion disk emission is less variable on these time scales and its power density follows 1/f law, contributing to observed flux variation at low frequencies and low energies only. The kHz QPOs have the same origin as variability at lower frequencies - independent of the nature of the "clock", the actual luminosity modulation takes place on the NS surface. The boundary layer spectrum remains nearly constant during luminosity variations and can be represented by the Fourier frequency resolved spectrum. In the range of Mdot~(0.1-1)*Mdot_Edd it depends weakly on the global mass accretion rate and in the limit Mdot~Mdot_Edd is close to Wien spectrum with kT~2.4 keV. Its independence on the Mdot lends support to the suggestion by Inogamov & Sunyaev (1999) that the boundary layer is radiation pressure supported. Based on the knowledge of the boundary layer spectrum we attempt to relate the motion along the Z-track to changes of physically meaningful parameters. Our results suggest that the contribution of the boundary layer to the observed emission decreases along the Z-track from conventional ~50% on the horizontal branch to a rather small number on the normal branch. This decrease can be caused, for example, by obscuration of the boundary layer by the geometrically thickened accretion disk at Mdot~Mdot_Edd. Alternatively, this can indicate significant change of the structure of the accretion flow at Mdot~Mdot_Edd and disappearance of the boundary layer as a distinct region of the significant energy release associated with the NS surface.
Astronomische Nachrichten, 326, No.9, p.812 (2005)
References in corpus (10)
- Millisecond Oscillations in X-Ray Binaries
- Simultaneous X-ray and gamma-ray observations of Cyg X-1 in the hard state by Ginga and OSSE
- Accretion Disk Boundary Layers Around Neutron Stars: X-ray Production in Low-Mass X-ray Binaries
- Boundary layer, accretion disk and X-ray variability in luminous LMXBs
- Detection of a Hard Tail in the X-ray Spectrum of the Z Source GX 349+2
- The broad band X-ray/hard X-ray spectra of accreting neutron stars
- Frequency resolved spectroscopy of Cyg X-1: fast variability of the reflected emission in the soft state
- Energy Release During Disk Accretion onto a Rapidly Rotating Neutron Star
- The X-ray Spectrum of Cyg X-2
- The spectra of accretion discs in low-mass X-ray binaries
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