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SGR 1935+2154
SGR 1935+2154 (or SGR J1935+2154) is a soft gamma repeater (SGR) and ancient stellar remnant, in the constellation Vulpecula, originally discovered in 2014 by the Neil Gehrels Swift Observatory. Currently, the SGR-phenomena and the related anomalous X-ray pulsars (AXP) are explained as arising from magnetars.
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