ATLAS J1138-5139 is a 28-minute binary of a 1.02-solar-mass and a 0.24-solar-mass white dwarf, the first candidate Type Ia supernova progenitor predicted to be detectable by LISA on its own.
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A gravitational wave detectable candidate Type Ia supernova progenitor
ATLAS J1138-5139 is a 28-minute binary of a 1.02-solar-mass and a 0.24-solar-mass white dwarf, the first candidate Type Ia supernova progenitor predicted to be detectable by LISA on its own.