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Cosmic Helium Production

Published online by Cambridge University Press:  05 March 2013

Chris Flynn
Chris Flynn*
Affiliation:
Centre for Astrophysics Supercomputing, Swinburne University, Hawthorn VIC 3122, Australia
*
3 E-mail: cflynn@oj287.astro.utu.fi
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Abstract

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K-dwarfs are very long lived, slowly evolving stars, so that their present day helium Y and metal content (metallicity Z) is essentially the same as when they were born. K-dwarfs thus contain a fossil record of the amount of helium and metals which has been produced in successive stellar generations over the lifetime of the Galaxy. We here estimate the amount of helium compared to the amount of metals produced via stellar fusion (Δ Y/ΔZ). We use K-dwarfs in the Hipparcos catalogue for which accurate metallicities and luminosities are available. By including recently measured K-dwarfs with super-solar metallicities we are able to obtain a very significant improvement on previous studies. The best fitting value is ΔY/ΔZ = 2.4 ± 0.4 at the 68% confidence level. Values as low as 1 or as high as 4 are excluded with more than 99% confidence.

Keywords

Galaxy: abundancesGalaxy: evolution

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