A multiwavelength study of the radio source G296.7โ0.9: confirmation as a Galactic supernova remnant
A multiwavelength study of the radio source G296.7โ0.9: confirmation as a Galactic supernova remnant
We present a multiwavelength study of the radio source G296.7โ0.9. This source has a bilateral radio morphology, a radio spectral index of โ0.5 ยฑ 0.1, sparse patches of linear polarization and thermal X-rays with a bright arc near the radio boundary. Considering these characteristics, we conclude that G296.7โ0.9 is a โฆ