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    Article

    A measurement of the equation of state of carbon envelopes of white dwarfs

    White dwarfs represent the final state of evolution for most stars1–3. Certain classes of white dwarfs pulsate4,5, leading to observable brightness variations, and analysis of these variations with theoretical st...

    Andrea L. Kritcher, Damian C. Swift, Tilo Döppner, Benjamin Bachmann… in Nature (2020)