Astronomers Confirm First Pair of Sibling Supernovae Hidden in Jellyfish Nebula
Astronomers have confirmed the first evidence of a binary star system where both stars exploded as supernovae, with their remnants found in the Jellyfish Nebula, also known as IC 443. This discovery, published in Nature Communications, resolves a long-standing gap in stellar evolution theory. The research, led by a Stanford team, utilized 16 years of gamma-ray data from NASA's Fermi space telescope, along with X-ray, infrared, ultraviolet, and radio observations. The findings show that the remnants, IC 443 and G189.6+3.3, were originally gravitational companions. This confirmation was achieved through multiwavelength evidence and simulations of one million binary systems, with a statistical test showing the odds of a chance alignment are less than one in 1,000.