Exploding dwarf
What starts as an ordinary binary star ends up as a white dwarf, detonating because of mass transfer from its red giant companion: a Type Ia supernova.
Credit:NASA/ESA/A. Feild (STScI), design und mehr
What starts as an ordinary binary star ends up as a white dwarf, detonating because of mass transfer from its red giant companion: a Type Ia supernova.
Credit:NASA/ESA/A. Feild (STScI), design und mehr