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zeige Details Porter, N. A. Cosmic-ray emission from Cygnus X-3
in: Nature . - London [u.a.] : Nature Publising Group, ISSN 1476-4687, Vol. 312, No. 5992 (1984), p. 347-348
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1984
Recent observations1,2 of the X-ray binary source Cygnus X-3 have revealed a flux of ultra-high energy γ rays. Other observations and subsequent models suggest that Cyg X-3 may be a dominant source of galactic high-energy cosmic rays. Here I investigate whether it is possible to escape this conclusion with a model in which most of the energy of accelerated particles at the source is emitted as curvature radiation (that is, radiation emitted by particles travelling on curved paths in a magnetic field so strong that synchrotron radiation is suppressed). I conclude that such a model is not consistent with the observations.
beteiligte Personen: Porter, N. A.
Format: Elektronisch
Erschienen: 1984.
Serie: Nature Archives 1869 - 2007 [Dig. Serial]
Schlagwörter:
URL: http://dx.doi.org/10.1038/312347a0

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