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Understanding the processes within compact stars hinges on astrophysical observations. A recent study reported on the central object in the HESS J1731-347 supernova remnant (SNR), estimating a mass of $M=0.77_{-0.17}^{+0.20} \ M_{\odot}$ and a radius
Externí odkaz:
http://arxiv.org/abs/2411.17234
