Hostname: page-component-745bb68f8f-v2bm5 Total loading time: 0 Render date: 2025-01-13T10:46:48.481Z Has data issue: false hasContentIssue false
  • English
  • Français

The Evolution of 4He and LiBeB

Published online by Cambridge University Press:  25 May 2016

Keith A. Olive
Keith A. Olive*
Affiliation:
Theoretical Physics Institute, School of Physics and Astronomy, University of Minnesota, Minneapolis MN 55455, USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Our understanding of the evolution of 4He and 7Li depends critically on the available data for these two elements at low metallicity. In particular, the degree to which there is a slope in an abundance vs metallicity regression can help determine the evolution of He, C, N, and O in dwarf galaxies in the case of 4He, and cosmic-ray induced nucleosynthesis of LiBeB in our own galaxy in the case of 7Li. Recent data and their implications will be discussed.

Type
7. Evolution of the Light Elements
Information
Symposium - International Astronomical Union , Volume 198: The Light Elements and their Evolution , 2000 , pp. 547 - 557
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

Alonso, A., Arribas, S., & Martinez-Roger, C. 1996a, A & AS, 117, 227 Google Scholar
Alonso, A., Arribas, S., & Martinez-Roger, C. 1996b, A & A, 313, 873 Google Scholar
Axer, M., Fuhrmann, K., & Gehren, T. 1994, A & A, 291, 895 Google Scholar
Boesgaard, A.M., King, J.R., Deliyannis, C.P., & Vogt, S.S. 1999a, AJ, 117, 492 Google Scholar
Boesgaard, A.M., Deliyannis, C.P., King, J.R., Ryan, S.G., Vogt, S.S., & Beers, T.C. 1999b, AJ, 117, 1549 Google Scholar
Bonifacio, P. & Molaro, P. 1997, MNRAS, 285, 847 Google Scholar
Bykov, A.M. 1999, in “LiBeB, cosmic rays and related X-and Gamma- Rays”, eds. Ramaty, et al., ASP, Vol. 171, p. 146 Google Scholar
Cassé, M., Lehoucq, R., & Vangioni-Flam, E. 1995, Nature, 373, 38 Google Scholar
Fields, B. D., Kainulainen, K., Olive, K. A., & Thomas, D. 1996, New Astron., 1, 77 Google Scholar
Fields, B.D. & Olive, K.A. 1998, ApJ, 506, 177 Google Scholar
Fields, B.D. & Olive, K.A. 1999, ApJ, 516, 797 Google Scholar
Fields, B.D. & Olive, K.A. 1999, New Astron., 4, 255 Google Scholar
Fields, B.D., Olive, K.A., Vangioni-Flam, E. & Cassé, M. 2000, astro-ph/9911320.Google Scholar
García-López, R.J., et al., Ap.J. 500 (1998)Google Scholar
Israelian, G., García-López, R.J., & Rebolo, R. 1998, ApJ, 507, 805 Google Scholar
Izotov, Y.I. & Thuan, T.X. 1998, ApJ, 500, 188.Google Scholar
Izotov, Y.I., Thuan, T.X., & Lipovetsky, V.A. 1994 ApJ 435, 647 CrossRefGoogle Scholar
Izotov, Y.I., Thuan, T.X., & Lipovetsky, V.A. 1997, ApJS, 108, 1 CrossRefGoogle Scholar
Meneguzzi, M., Audouze, J., & Reeves, H. 1971, A&A, 15, 337 Google Scholar
Olive, K.A., Steigman, G. & Skillman, E.D. 1997, ApJ, 483, 788 Google Scholar
Olive, K.A. & Skillman, E. 2000, in preparation.Google Scholar
Pagel, B.E.J., Simonson, E.A., Terlevich, R.J. & Edmunds, M. 1992, MNRAS, 255, 325 CrossRefGoogle Scholar
Ramaty, R., Kozlovsky, B., Lingenfelter, R.E., & Reeves, H. 1997, ApJ, 488, 730 Google Scholar
Ramaty, R., Scully, S., Lingenfelter, R. and Kozlovsky, B. 1999 (astro-ph/9909021) Google Scholar
Reeves, H., Fowler, W.A., & Hoyle, F. 1970, Nature, 226, 727 Google Scholar
Ryan, S.G., Beers, T.C., Olive, K.A., Fields, B.D., & Norris, J.E. 2000, ApJL, in press (astro-ph/9905211) Google Scholar
Ryan, S.G., Norris, J.E., & Beers, T.C. 1999, ApJ, 523, 654 Google Scholar
Skillman, E., & Kennicutt, 1993, ApJ, 411, 655 Google Scholar
Skillman, E., Terlevich, R.J., Kennicutt, R.C., Garnett, D.R., & Terlevich, E. 1994, ApJ, 431, 172 CrossRefGoogle Scholar
Spite, F. & Spite, M. 1982, A&A, 115, 357 Google Scholar
Vangioni-Flam, E., Cassé, M., Audouze, J., & Oberto, Y. 1990, ApJ, 364, 568 Google Scholar
Vangioni-Flam, E., Cassé, M., Fields, B.D., & Olive, K.A. 1996, ApJ, 468, 199 Google Scholar