Produced by: Manoj Kumar
A newly discovered binary star features a white dwarf with an extreme 38.7 MG magnetic field, siphoning gas from its tiny companion.
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This white dwarf is relentlessly stripping its companion star, creating intense radiation and violent stellar outbursts.
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The two stars are locked in a death spiral, orbiting each other in just over an hour—one of the fastest known cataclysmic variables.
With no accretion disk, the white dwarf’s magnetic field channels matter directly onto its poles, unleashing dazzling cyclotron radiation.
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Scientists predict this system may generate gravitational waves detectable by future space-based observatories like LISA.
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This white dwarf’s magnetic field is strong enough to reshape gas flows, creating a cosmic spectacle of swirling plasma.
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As these stars orbit ever closer, their violent interactions could help scientists unravel the fate of extreme binary systems.
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When the LISA mission launches in 2035, this star system may become one of the first new sources of gravitational waves ever detected in space.
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This rare system provides a perfect testbed for studying white dwarf evolution, magnetic field physics, and the future of binary stars.
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