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• W2564395894 abstract "We use a seismic diagnostic, based on the derivative of the phase shift of the acoustic waves reflected by the surface, to probe the outer layers of the star HD 49933. This diagnostic is particularly sensitive to partial ionization processes occurring above the base of the convective zone. The regions of partial ionization of light elements, hydrogen and helium, have well-known seismological signatures. In this work, we detect a different seismic signature in the acoustic frequencies, which we showed to correspond to the location where the partial ionization of heavy elements occurs. The location of the corresponding acoustic glitch lies between the region of the second ionization of helium and the base of the convective zone, approximately 5 per cent below the surface of the stars." @default.
• W2564395894 created "2017-01-06" @default.
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• W2564395894 date "2016-12-13" @default.
• W2564395894 modified "2023-10-01" @default.
• W2564395894 title "TheCoRoTtarget HD 49933: a possible seismic signature of heavy elements ionization in the deep convective zone" @default.
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• W2564395894 doi "https://doi.org/10.1093/mnras/stw3241" @default.
• W2564395894 hasPublicationYear "2016" @default.
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