X-ray detection of astrospheres around three main-sequence stars and their mass-loss rates

LEO's

Nature Astronomy, Published online: 12 April 2024; doi:10.1038/s41550-024-02222-x

Stellar winds of main-sequence stars are extremely important for the evolution of both stars and planets, yet they are challenging to detect. Here a detection of charge-exchange X-ray emission from stellar winds from three main-sequence stars is presented, along with derived mass-loss rates.

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