Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/171256
Title: Binaries with the eyes of CTA
Author: Paredes i Poy, Josep Maria
Bednarek, W.
Bordas, P.
Bosch-Ramon, V.
De Cea del Pozo, E.
Dubus, G.
Funk, S.
Hadasch, D.
Khangulyan, D.
Markoff, S.
Moldón Vara, Francisco Javier
Munar i Adrover, Pere
Nagataki, S.
Naito, T.
De Naurois, M.
Pedaletti, G.
Reimer, O.
Ribó Gomis, Marc
Szostek, A.
Terada, Y.
Torres, D.F.
Zabalza de Torres, Víctor
Zdziarski, A.A. for the CTA Consortium
Keywords: Astronomia de raigs gamma
Estels binaris de raigs X
Telescopis
Observacions astronòmiques
Gamma ray astronomy
X-ray binaries
Telescopes
Astronomical observations
Issue Date: Mar-2013
Publisher: Elsevier B.V.
Abstract: The binary systems that have been detected in gamma rays have proven very useful to study high-energy processes, in particular particle acceleration, emission and radiation reprocessing, and the dynamics of the underlying magnetized flows. Binary systems, either detected or potential gamma-ray emitters, can be grouped in different subclasses depending on the nature of the binary components or the origin of the particle acceleration: the interaction of the winds of either a pulsar and a massive star or two massive stars; accretion onto a compact object and jet formation; and interaction of a relativistic outflow with the external medium. We evaluate the potentialities of an instrument like the Cherenkov telescope array (CTA) to study the non-thermal physics of gamma-ray binaries, which requires the observation of high-energy phenomena at different time and spatial scales. We analyze the capability of CTA, under different configurations, to probe the spectral, temporal and spatial behavior of gamma-ray binaries in the context of the known or expected physics of these sources. CTA will be able to probe with high spectral, temporal and spatial resolution the physical processes behind the gamma-ray emission in binaries, significantly increasing as well the number of known sources. This will allow the derivation of information on the particle acceleration and emission sites qualitatively better than what is currently available.
Note: Versió postprint del document publicat a: https://doi.org/10.1016/j.astropartphys.2012.09.004
It is part of: Astroparticle Physics, 2013, vol. 43, p. 301-316
URI: http://hdl.handle.net/2445/171256
Related resource: https://doi.org/10.1016/j.astropartphys.2012.09.004
ISSN: 0927-6505
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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