ASKAP$-$EMU Discovery of “Raspberry”: a new Galactic SNR Candidate G308.73+1.38
Sanja Lazarevi’c, Miroslav D. Filipovi’c, B"arbel S. Koribalski, Zachary J. Smeaton, Andrew M. Hopkins, Rami Z. E. Alsaberi, Velibor Velovi’c, Brianna D. Ball, Roland Kothes, Denis Leahy, Adriano Ingallinera
arXiv:2405.03733v1 Announce Type: new
Abstract: We report the ASKAP discovery of a new Galactic supernova remnant (SNR) candidate G308.73+1.38, which we name Raspberry. This new SNR candidate has an angular size of 20.7 arcmin $times$ 16.7 arcmin, and we measure a total integrated flux of 407$pm$50 mJy. We estimate Raspberry’s most likely diameter of 10$-$30 pc which would place it at a distance of 3$-$5 kpc, on the near side of the Milky Way’s Scutum$-$Centaurus Arm. We also find a Stokes$-$V point source close to the centre of Raspberry with a $sim$5$sigma$ significance. This point source may be the remaining compact source, a neutron star, or possibly a pulsar, formed during the initial supernova event.arXiv:2405.03733v1 Announce Type: new
Abstract: We report the ASKAP discovery of a new Galactic supernova remnant (SNR) candidate G308.73+1.38, which we name Raspberry. This new SNR candidate has an angular size of 20.7 arcmin $times$ 16.7 arcmin, and we measure a total integrated flux of 407$pm$50 mJy. We estimate Raspberry’s most likely diameter of 10$-$30 pc which would place it at a distance of 3$-$5 kpc, on the near side of the Milky Way’s Scutum$-$Centaurus Arm. We also find a Stokes$-$V point source close to the centre of Raspberry with a $sim$5$sigma$ significance. This point source may be the remaining compact source, a neutron star, or possibly a pulsar, formed during the initial supernova event.

Comments are closed, but trackbacks and pingbacks are open.