Observation of Kes 27: A Typical Mixed-Morphology SNR
نویسندگان
چکیده
منابع مشابه
Observation of AXP 1 E 1841 - 045 in SNR Kes 73
Anomalous X-ray pulsars (AXPs) are thought to be magnetars, which are neutron stars with ultra strong magnetic field of 1014–1015 G. Their energy spectra below ∼10 keV are modeled well by two components consisting of a blackbody (BB) (∼0.4 keV) and rather steep power-law (POW) function (photon index ∼2-4). Kuiper et al.(2004) discovered hard X-ray component above ∼10 keV from some AXPs. Here, w...
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ژورنال
عنوان ژورنال: Publications of the Astronomical Society of Japan
سال: 2002
ISSN: 0004-6264,2053-051X
DOI: 10.1093/pasj/54.2.229