Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/50795
Title: The 2010 May Flaring Episode of Cygnus X-3 in Radio, X-rays, and γ-rays
Author: Williams, Peter K. G.
Tomsick, John A.
Bodaghee, Arash
Bower, Geoffrey C.
Pooley, G.
Pottschmidt, Katja
Rodriguez, Jérôme
Wilms, Jörn
Migliari, Simone
Trushkin, Sergei A.
Keywords: Forats negres (Astronomia)
Estels binaris de raigs X
Jets (Astrofísica)
Astrofísica
Black holes (Astronomy)
X-ray binaries
Astrophysical jets
Astrophysics
Issue Date: Jun-2011
Publisher: Institute of Physics (IOP)
Abstract: In 2009, Cygnus X-3 (Cyg X-3) became the first microquasar to be detected in the GeV γ-ray regime, via the satellites Fermi and AGILE. The addition of this new band to the observational toolbox holds promise for building a more detailed understanding of the relativistic jets of this and other systems. We present a rich data set of radio, hard and soft X-ray, and γ-ray observations of Cyg X-3 made during a flaring episode in 2010 May. We detect a ~3 day softening and recovery of the X-ray emission, followed almost immediately by a ~1 Jy radio flare at 15 GHz, followed by a 4.3σ γ-ray flare (E > 100 MeV) ~1.5 days later. The radio sampling is sparse, but we use archival data to argue that it is unlikely the γ-ray flare was followed by any significant unobserved radio flares. In this case, the sequencing of the observed events is difficult to explain in a model in which the γ-ray emission is due to inverse Compton scattering of the companion star's radiation field. Our observations suggest that other mechanisms may also be responsible for γ-ray emission from Cyg X-3.
Note: Reproducció del document publicat a: http://dx.doi.org/10.1088/2041-8205/733/2/L20
It is part of: Astrophysical Journal, 2011, vol. 733, num. 2, p. 1-6
Related resource: http://dx.doi.org/10.1088/2041-8205/733/2/L20
URI: http://hdl.handle.net/2445/50795
ISSN: 0004-637X
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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