In about 5 to 8 billion years, our sun is expected to evolve into a white dwarf—an extremely dense, Earth-sized stellar remnant that has exhausted its fuel and shed its outer layer. But while our sun is a solitary star, research over the past 15 years has demonstrated that binary or multi-star systems are far more common than astronomers once thought. When a dense and compact remnant like a white dwarf is involved in a binary system, it often “snatches away” material from its companion star. This process, called accretion, usually emits X-rays in what is considered a “signature” signal.
Now, scientists from the group of Ilaria Caiazzo, assistant professor at the Institute of Science and Technology Austria (ISTA), confirm the detection of an X-ray signal in not just one, but two isolated objects called Gandalf and Moon-Sized. Highly magnetic and rapidly rotating, these two objects are called “merger remnants” as they each formed as a result of a violent cosmic collision. By emitting X-rays in the absence of a companion, they now form a new class of their own.









