SGR 1935 2154

SGR 1935+2154 (or SGR J1935+2154) is a soft gamma repeater (SGR) that is an ancient stellar remnant, in the constellation Vulpecula, originally discovered

million Jy ms, was detected from the same area of sky as the magnetar SGR 1935+2154. Although it was thousands of times less intrinsically bright than previously

bursts (FRBs) and magnetars was suggested, based on observations of SGR 1935+2154, a likely magnetar located in the Milky Way galaxy. As of July 2021[update]

magnetar SGR 1935+2154". The Astronomer's Telegram. Retrieved 1 May 2020. Younes, George; et al. (28 April 2020). "Burst forest from SGR 1935+2154 as detected

October 2024). "GTC optical/NIR upper limits and NICER X-ray analysis of SGR J1935+2154 for the outburst in 2022". arXiv:2410.00635 [astro-ph.HE]. Kurban, Abdusattar;