Seismological measurement of stellar ages

Details Seismological measurement of stellar ages Seismological measurement of stellar ages

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987natur.326..257g&link_type=abstract

Nature (ISSN 0028-0836), vol. 326, March 19, 1987, p. 257-259.

Physics

58

Acoustic Frequencies, Main Sequence Stars, Seismology, Stellar Evolution, Stellar Oscillations, Abundance, Frequency Measurement, Stellar Structure

Scientific paper

Accurate measurements of stellar acoustic oscillation frequencies, which are likely to be obtained in the coming years, will provide important new data enabling us to diagnose the internal structure of stars. The ages of main-sequence stars are likely to be determined to a higher precision than has been possible in the past and much more accurate estimates of the total heavy-element abundances should be possible.

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