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- W2520044319 abstract "Supernova Remnant RX J1713.7-3946 emits synchrotron X-rays and very high energy $gamma$-rays. Recently, thermal X-ray line emission is detected from ejecta plasma. CO and HI observations indicate that a highly inhomogeneous medium surrounding the SNR. It is interacting with dense molecular clouds in the northwest and the southwest of the remnant. The origin of the $gamma$-ray emission from RX J1713.7-3946 is still uncertain. Detection of rapid variability in X-ray emission from RX J1713.7-3946 indicates the magnetic field $B$ $sim$ mG. In this work, we investigate the time variation in X-ray flux, luminosity and photon index of RX J1713.7-3946. For this investigation, we study the northwest part of the remnant using Suzaku data in 2006 and 2010. We present preliminary results based on our analysis and interpretations about these X-ray time variability." @default.
- W2520044319 created "2016-09-23" @default.
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- W2520044319 date "2016-09-13" @default.
- W2520044319 modified "2023-09-27" @default.
- W2520044319 title "Searching for the Time Variation in Supernova Remnant RX J1713.7-3946" @default.
- W2520044319 hasPublicationYear "2016" @default.
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