A jet model for black-hole X-ray sources

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dc.creatorKylafis, N. D.
dc.creatorPapadakis, I. E.
dc.creatorReig, P.
dc.date2007-02-27
dc.date.accessioned2026-07-07T10:21:52Z
dc.date.available2026-07-07T10:21:52Z
dc.descriptionA jet model for Galactic black-hole X-ray binaries will be presented that appears to explain several observational characteristics. In particular, it explains the energy spectrum from radio to hard X-rays, the time-lags as a function of Fourier frequency, the increase of the variability amplitude (QPO and high frequency) with increasing photon energy, and the narrowing of the autocorrelation function with increasing photon energy. On the other hand, there are additional observational constraints that no model has tried to explain yet. It is important that we all try to address these constraints if we are to make any progress in understanding black-hole X-ray sources
dc.descriptionI Microquasar Workshop: Microquasars and Beyond, September 18-22 2006
dc.identifierhttps://arxiv.org/abs/astro-ph/0702710
dc.identifierhttp://arxiv.org/abs/astro-ph/0702710
dc.identifierPoSMQW6:039,2006
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175317
dc.subjectAstrophysics
dc.titleA jet model for black-hole X-ray sources
dc.typetext

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