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 identified a hidden white dwarf companion as the source of extreme X-rays from the naked-eye star Gamma Cassiopeiae. Observations from Japan's XRISM space telescope revealed the companion's orbital motion through shifting plasma velocities. The discovery confirms a long-predicted class of binary star systems.

Astronomers have identified massive rings of plasma around young M dwarf stars that function as built-in monitors for stellar space weather. These structures, presented at the American Astronomical Society meeting, could help assess conditions for habitable planets orbiting these common stars. The findings come from research by Carnegie's Luke Bouma and Moira Jardine of the University of St Andrews.

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Astronomers have uncovered evidence that a black hole and neutron star merged while following an unusual oval-shaped orbit, challenging expectations of circular paths in such events. The discovery comes from a reanalysis of gravitational wave data from the event known as GW200105. This finding suggests the system formed in a dynamic stellar environment.

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