Astrophysicists have found that a recently-discovered transient radio source, ILT J110160.52+552119.62, whose roughly minute-long pulses arrive with a periodicity of 125.5 min, is an red dwarf-white dwarf binary system with an orbital period that matches the period of the radio pulses, which are observed when the two stars are in conjunction. Artistic illustration showing the radio pulses emitted by the binary star system: a white dwarf in orbit...
