A light strange star in the remnant HESS J1731-347: Minimal consistency checks

Context: Recently, Doroshenko and collaborators reported a very low-mass compact star, Central Compact Object named XMMU J173203.3-344518 inside the supernova remnant HESS J1731-347. Its tiny mass is at odds with all calculations of minimum masses neutron stars generated by iron cores, therefore (and even if not compellingly) it has been suggested to be {\it strange star}. Besides mass, radius surface temperature have extracted from data, whole body information should ultimately reveal this object truly consistent an exotic composition. Aims: To understand status in J1731-347 within existing models stars, including its prompt formation. Methods: The obtained on are compared theoretical performed usual using General Relativity as assumed theory gravitation handful cooling scenarios. A qualitative discussion showing consistency strange-matter driven scenario star provided. Results: We found that fits same quark recently employed explain radii NICER objects PSR J040+6620 J0030+0451, which both quantities were simultaneously determined. It also remarkable find simple devised $30\text{ yr}$ ago superconducting quarks provides overall good explanation temperature. Conclusions: conclude into ``strange star'' heavier can belong class constitute homogeneous type self-bound produced Nature.