White dwarf binary traced as source of repeating cosmic signals

Astronomers have identified a rare stellar pair as the origin of long-period radio transients, mysterious repeating signals detected in the Milky Way. The system features a white dwarf drawing material from a red dwarf companion.

An international team led by researchers at the University of Sydney made the discovery with CSIRO's ASKAP radio telescope. The system, named ASKAP J1745−5051, produces radio waves and X-rays that repeat every 1.4 hours as the stars orbit each other. Lead author Kovi Rose said the findings confirm the source as a cataclysmic variable, or accreting white dwarf star.

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Astronomers have identified the source of unusual X-rays from the bright star gamma-Cas as a hidden white dwarf companion siphoning material from it. High-resolution data from the XRISM space mission confirmed that the emissions arise from matter heating up as it falls onto the unseen star. The discovery ends a puzzle that has intrigued scientists since the 1970s.

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Astronomers have confirmed four white dwarf stars previously hidden in binary systems within 65 light-years of Earth. One system, located just 25 light-years away, ranks as the ninth closest known white dwarf to the Sun.

Researchers using the DAMPE space telescope have identified a shared spectral softening in cosmic rays across multiple particle types. The pattern appears at a rigidity of about 15 teraelectron-volts for protons through iron nuclei. This finding, published in Nature, offers new insight into how these high-energy particles behave in the galaxy.

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Researchers have created an artificial intelligence system to analyze millions of Type Ia supernovae using imaging data alone. The approach could sharpen estimates of cosmic distances and probe the nature of dark energy. It is designed for upcoming large-scale surveys by the Vera C. Rubin Observatory.

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