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Light Element Evolution at the Solar Neighborhood

Published online by Cambridge University Press:  25 May 2016

Andreu Alibés ,
Javier Labay  and
Ramon Canal
Andreu Alibés
Affiliation:
Departament d’Astronomia i Meteorologia, Universitat de Barcelona, C/Martí i Franquès 1, 08028 Barcelona, Spain
Javier Labay
Affiliation:
Departament d’Astronomia i Meteorologia, Universitat de Barcelona, C/Martí i Franquès 1, 08028 Barcelona, Spain
Ramon Canal
Affiliation:
Departament d’Astronomia i Meteorologia, Universitat de Barcelona, C/Martí i Franquès 1, 08028 Barcelona, Spain

Abstract

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We present the Light Element Evolution resulting from our new Chemical Evolution model. The LiBeB evolution is correctly fitted by taking into account several sources: Big Bang, Galactic Cosmic Ray Nucleosynthesis, the ν-process, novae and AGB and C-stars.

Type
7. Evolution of the Light Elements
Information
Symposium - International Astronomical Union , Volume 198: The Light Elements and their Evolution , 2000 , pp. 563 - 564
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

Abia, C., Isern, J., & Canal, R. 1993, A&A, 275, 96 Google Scholar
Chiappini, C., Matteucci, F., & Gratton, R. 1997, ApJ, 477, 765 Google Scholar
José, J., & Hernanz, M. 1998, ApJ, 494, 680 CrossRefGoogle Scholar
Matteucci, F., D'Antona, F., & Timmes, F.X. 1995, A&A, 303, 460 Google Scholar
Ramaty, R., Kozlovsky, B., Lingenfelter, R.E., & Reeves, H. 1997, ApJ, 488, 730 CrossRefGoogle Scholar
Romano, D., Matteucci, F., Molaro, P., & Bonifacio, P. 1999, A&A, 352, 117 Google Scholar
Woosley, S.E., & Weaver, T.A. 1995, ApJS, 101, 181 Google Scholar