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dc.contributor.author | Reig Torres, Pablo | |
dc.contributor.author | Kylafis, N.D. | |
dc.contributor.author | Giannios, Dimitrios | |
dc.date.accessioned | 2010-07-30T11:03:54Z | |
dc.date.available | 2010-07-30T11:03:54Z | |
dc.date.issued | 2003 | |
dc.identifier.citation | REIG TORRES, Pablo ; Kylafis, N.D. ; Giannios, Dimitrios, 2003, Energy and time-lag spectra of galactic black-hole X-ray sources in the low/hard state, Astronomy and Astrophysics, vol. 403, no. 1, p. L15-L18 | en |
dc.identifier.uri | http://hdl.handle.net/10550/16741 | |
dc.description.abstract | Most, probably all, accreting binaries that are believed to contain a black-hole emit radio waves when they are in the low/hard state. Whenever this radio emission has been resolved, a jet-like structure has become apparent. We propose that Compton upscattering of low-energy photons in the jet can explain both the energy spectra and the time lags versus Fourier frequency observed in the low/hard state of black-hole systems. The soft photons originate in the inner part of the accretion disk. We have performed Monte Carlo simulations of Compton upscattering in a jet and have found that for a rather wide range of values of the parameters we can obtain power-law high-energy X-ray spectra with photon-number index in the range 1.5–2 and power-law time lags versus Fourier frequency with index ∼0.7. The black-hole source Cyg X-1 in the low/hard state is well described by our model. | en |
dc.language.iso | en | en |
dc.title | Energy and time-lag spectra of galactic black-hole X-ray sources in the low/hard state | en |
dc.type | journal article | es_ES |
dc.subject.unesco | UNESCO::ASTRONOMÍA Y ASTROFÍSICA | en |
dc.subject.unesco | UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia | en |
dc.identifier.doi | 10.1051/0004-6361:20030449 | en |
dc.type.hasVersion | VoR | es_ES |
dc.identifier.url | http://www.aanda.org/index.php?option=article&access=standard&Itemid=129&url=/articles/aa/pdf/2003/19/aafa313.pdf | en |