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Interstellar Lithium as a probe of the primordial abundance
Published online by Cambridge University Press: 23 April 2010
Abstract
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The cosmic abundance of lithium continues to represent a conundrum, as predictions from BBN theory are inconsistent with measurements in the atmospheres of the lowest-metallicity stars. While there are worries that modifications of the stellar Li abundances may play a role in this discrepancy, no satisfactory solution has yet been found. We suggest an alternate approach to studying the cosmic abundance of Li: measurements of interstellar gas-phase Li in low-metallicity environments.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 5 , Symposium S268: Light Elements in the Universe , November 2009 , pp. 335 - 336
- Copyright
- Copyright © International Astronomical Union 2010
References
Baade, D., Cristiani, S., Lanz, T., Malaney, R. A., Sahu, K. S., & Vladilo, G. 1991, A&A, 251, 253Google Scholar
Cyburt, R. H., Fields, B. D., & Olive, K. A. 2009, J. Cosmology & Astroparticle Physics, 11, 012Google Scholar
Vidal-Madjar, A., Andreani, P., Cristiani, S., Ferlet, R., Lanz, T., & Vladilo, G. 1987, A&A, 177, L17Google Scholar
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