HESS J1616−508: likely to be powered by PSR J1617−5055
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چکیده
منابع مشابه
HESS J 1616 – 508 : likely powered by PSR J 1617 – 5055
HESS J1616–508 is one of the brightest emitters in the TeV sky. Recent observations with the IBIS/ISGRI telescope on board the INTEGRAL spacecraft have revealed that a young, nearby and energetic pulsar, PSR J1617–5055, is a powerful emitter of soft γ-rays in the 20–100 keV domain. In this paper we present an analysis of all available data from the INTEGRAL, Swift, BeppoSAX and XMM-Newton teles...
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We observed the young energetic pulsar J1617−5055 with the Chandra ACIS detector for 60 ks. In addition to the pulsar, the X-ray images show a faint pulsar-wind nebula (PWN) seen up to ∼ 1′ from the pulsar. Deconvolution and reconstruction of the image reveal a brighter compact PWN component of ∼ 1′′ size, possibly with a jet-torus morphology. The PWN spectrum fits an absorbed power-law (PL) mo...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2007
ISSN: 0035-8711
DOI: 10.1111/j.1365-2966.2007.12168.x