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Advanced filters: Author: Andry Rajoelimanana Clear advanced filters

  • Accretion onto the surface of a white dwarf typically generates supersoft X-ray emission and broad emission lines due to nuclear fusion. ASASSN-16oh exhibits no visible broad lines, implying there is no surface fusion, and instead, a belt around the dwarf called a spreading layer is the source of the supersoft X-ray emission.

    • Thomas J. Maccarone
    • Thomas J. Nelson
    • Krzysztof Ulaczyk
    Research
    Nature Astronomy
    Volume: 3, P: 173-177