Chemical composition of evolved stars in the open cluster IC 4651★ (Q57672675)

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Gražina Tautvaišienė

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Raffaele Gratton

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Angela Bragaglia

Monthly Notices of the Royal Astronomical Society

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language of work or name

English

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publication date

8 March 2011

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number of pages

8 page

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based on heuristic

inferred from page(s)

published in

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SIMBAD

volume

413

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SIMBAD

issue

3

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page(s)

2199–2206

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Deriving temperature, mass, and age of evolved stars from high-resolution spectra. Application to field stars and the open cluster IC 4651

SIMBAD

cites work

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Deep mixing of 3He: reconciling Big Bang and stellar nucleosynthesis.

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Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 M?, and from Z=0.0004 to 0.03

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Critical tests of stellar evolution in open clusters

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Chemical composition of clump stars in the open cluster NGC 6134★

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Detailed chemical composition of the open cluster IC 4651: The iron peak, $\mathsf{\alpha}$ elements, and Li

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Metal Abundances of Red Clump Stars in Open Clusters. I. NGC 6819

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Thermohaline mixing in evolved low-mass stars

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Iron abundances from high-resolution spectroscopy of the open clusters NGC 2506, NGC 6134, and IC 4651

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