Definition
Isochrones are theoretical tracks in the Hertzsprung-Russell diagram (HRD) defining the position occupied by stars of a given age. Isochrones are used to determine the age of a stellar population, typically a star cluster: on an isochrone, the smaller mass stars may still lie on the main sequence, while the higher mass stars have already left the main sequence to become red giants. The determination of the mass of the stars that are precisely at the turnoff from the main sequence gives the age of the cluster.
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© 2014 Springer-Verlag Berlin Heidelberg
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Ekström, S. (2014). Isochrone. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_817-4
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DOI: https://doi.org/10.1007/978-3-642-27833-4_817-4
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Publisher Name: Springer, Berlin, Heidelberg
Online ISBN: 978-3-642-27833-4
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