
There are several ways in which the supernova can form. In the case of these two supernovae, the explosions evolved from two independent binary star systems in which the stellar remnant of a Sun-like star, known as a white dwarf, was collecting material from its companion star.
if (jQuery ("# crm_srl-th_scienze_d_mh2_1"). is (": visible")) {console.log ("Edinet ADV adding zone: tag crm_srl-th_scienze_d_mh2_1 slot id: th_scienze_d_mh2"); } Feeding on its partner, the white dwarf has absorbed material until it reaches a maximum mass. At this point, the star collapsed inward before exploding outward in a brilliant supernova. Two of these events have been spotted in NGC 3583, and although they are not visible, we can still admire the frightening symmetry of the galaxy.