| Reference Type | Journal (article/letter/editorial) |
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| Title | The boron-to-beryllium ratio in halo stars - A signature of cosmic-ray nucleosynthesis in the early Galaxy |
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| Journal | The Astrophysical Journal |
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| Authors | Walker, T. P. | Author |
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| Steigman, G. | Author |
| Schramm, D. N. | Author |
| Olive, K. A. | Author |
| Fields, B. | Author |
| Year | 1993 (August) | Volume | 413 |
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| Publisher | IOP Publishing |
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| DOI | doi:10.1086/173025Search in ResearchGate |
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| Generate Citation Formats |
| Mindat Ref. ID | 3333459 | Long-form Identifier | mindat:1:5:3333459:2 |
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|
| GUID | 0 |
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| Full Reference | Walker, T. P., Steigman, G., Schramm, D. N., Olive, K. A., Fields, B. (1993) The boron-to-beryllium ratio in halo stars - A signature of cosmic-ray nucleosynthesis in the early Galaxy. The Astrophysical Journal, 413. 562pp. doi:10.1086/173025 |
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| Plain Text | Walker, T. P., Steigman, G., Schramm, D. N., Olive, K. A., Fields, B. (1993) The boron-to-beryllium ratio in halo stars - A signature of cosmic-ray nucleosynthesis in the early Galaxy. The Astrophysical Journal, 413. 562pp. doi:10.1086/173025 |
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| In | (1993) The Astrophysical Journal Vol. 413. IOP Publishing |
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These are possibly similar items as determined by title/reference text matching only.