Astronomers trace mystery radio signals back to cosmic odd couple of white dwarf and sun-like star
AI-summarised brief · reviewed before publication
Astronomers have identified the source of mysterious radio pulses in the binary system GPM J071507−114153, located about 5,000 light‑years away. The system consists of a rapidly spinning white dwarf and a sun‑like companion. Using the Murchison Widefield Array, MeerKAT, and Keck Observatory, researchers confirmed that the pulses originate near the white dwarf, the first clear evidence of this in a long‑period transient (LPT). The discovery also revealed stellar flares on the companion and a magnetic prominence, offering new insight into LPT mechanisms.
💡 Why It Matters
- · Pinpointing the white dwarf as the pulse source resolves a long‑standing ambiguity in LPT studies, sharpening models of stellar magnetism and binary evolution.