In the current situation, Lu Chen also had no solution for the time being and could only watch as the quasi-star plundered his hydrogen gas.
When the quasi-star had plundered a constant star mass of high-temperature hydrogen gas, the temperature on the white dwarf star's surface, which had experienced a helium flash, suddenly soared, reigniting nuclear fusion reactions and beginning to emit a faint glow once again.
As more and more hydrogen was plundered, the nuclear fusion reaction on the surface of the quasi-star became increasingly intense. A large amount of luminous radiation burst forth, rapidly raising the temperature on the surface of the white dwarf star to over eight million degrees. At this temperature, the high-density white dwarf star began to gradually gasify, turning into carbon ions.
Because the ultra-high density white dwarf star was originally constructed from carbon atoms.
