SGR 1935+2154
id:
sgr-1935-2154-200-348977
title:
SGR 1935+2154
text:
SGR 1935+2154 is a soft gamma repeater (SGR) that is an 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. On 28 April 2020, this remnant about 30,000 light-years away in our Milky Way galaxy was observed to be associated with a very powerful radio pulse known as a fast radio burst or FRB, and a related x-ra
brand slug:
wiki
category slug:
encyclopedia
description:
Soft gamma repeater in the constellation Vulpecula
original url:
https://en.wikipedia.org/wiki/SGR_1935%2B2154
date created:
date modified:
2023-03-08T05:03:39Z
main entity:
{"identifier":"Q88697465","url":"https://www.wikidata.org/entity/Q88697465"}
image:
{"content_url":"https://upload.wikimedia.org/wikipedia/commons/6/6c/Artist%E2%80%99s_impression_of_a_fast_radio_burst_traveling_through_space_and_reaching_Earth.tif","width":5180,"height":3344}
fields total:
13
integrity:
15