dc.creatorReynoso, M. M.
dc.creatorChristiansen, H. R.
dc.creatorRomero, Gustavo Esteban
dc.date2008
dc.date2021-11-26T17:47:32Z
dc.date.accessioned2023-07-15T04:06:40Z
dc.date.available2023-07-15T04:06:40Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/128741
dc.identifierissn:0927-6505
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7468293
dc.descriptionWe discuss the gamma-ray absorption in the inner region of the microquasar SS433. Our investigation includes several contributions to the opacity of this system. They result from the ambient fields generated by the primary star, possibly an A-type supergiant, and a very extended disk around the black hole. Besides the sharp and dramatic absorption effect that occurs every time the star crosses the emission zone, we find in the UV photon field from the extended disk an important source of absorption for very high energy gamma-rays. This results in periodic gamma-ray observational signatures.
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.formatapplication/pdf
dc.format565-572
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectCiencias Astronómicas
dc.subjectGamma-rays: theory
dc.subjectX-rays: binaries
dc.subjectRadiation mechanisms: non-thermal
dc.subjectStars: winds
dc.subjectOutflows
dc.titleGamma-ray absorption in the microquasar SS433
dc.typeArticulo
dc.typePreprint


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