Asteroseismic ages from TESS calibrate [Y/Mg] and [C/N] chemical clocks, revealing a radially dependent [Y/Mg]-age relation that is steeper in the outer Galactic disc and flatter inward, with NLTE corrections and evolutionary stage accounting required for accuracy.
E., Phillip, C., Fleming, S
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TESS data yield a fast white-dwarf spin-down rate in V1405 Cas indicating a propeller regime, a previously unknown 1.36-day orbital period in V1716 Sco, and confirmed periods in V1674 Her, highlighting unexpected properties of accreting white dwarfs.
citing papers explorer
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Calibration of the [C/N] and [Y/Mg] chemical clocks with asteroseismic ages from the TESS space mission
Asteroseismic ages from TESS calibrate [Y/Mg] and [C/N] chemical clocks, revealing a radially dependent [Y/Mg]-age relation that is steeper in the outer Galactic disc and flatter inward, with NLTE corrections and evolutionary stage accounting required for accuracy.
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A TESS View of Post-Eruption Variability in the Novae V1405 Cas,V1716 Sco, and V1674 Her
TESS data yield a fast white-dwarf spin-down rate in V1405 Cas indicating a propeller regime, a previously unknown 1.36-day orbital period in V1716 Sco, and confirmed periods in V1674 Her, highlighting unexpected properties of accreting white dwarfs.