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- W2022206606 abstract "AX J2049.6+2939 is a compact source in the vicinity of the southern blow-up region of the Cygnus Loop super-nova remnant (Miyata 1998). This source is the brightest X-ray source found during the ASCA survey of the Cygnus Loop. The X-ray spectrum could be well fitted by a power-law function with an index of 2.1 ± 0.1. Timing analysis was performed and no coherent pulsation was found. Taking into account the X-ray properties, we conclude that AX J2049.6+2939 is either an AGN or a spin-powered pulsar. We again observed AX J2049.6+2939 with ASCA. The GIS count rate was a factor of 40 lower than that of the first ASCA observation. This suggests that AX J2049.6+2939 is not likely to be an ordinary rotation-powered pulsar. The X-ray intensity of the third ASCA observation is consistent with that of the second observation. The nature of AX J2049.6+2939 is still unclear and further observation with a wide energy band is strongly required." @default.
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- W2022206606 date "1999-08-01" @default.
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- W2022206606 title "The X-ray nature of AX J2049.6+2939" @default.
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- W2022206606 doi "https://doi.org/10.1002/1521-3994(199908)320:4/5<337::aid-asna337>3.0.co;2-o" @default.
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