Gamma-ray spectroscopy holds great promise for probing nucleosynthesis in individual stellar explosions via short-lived radioactivity, and for measuring current global Galactic nucleosynthesis with longer-lived radioactivity. The former case was realized first for a Type II supernova when both 56Co
โฆ LIBER โฆ
Gamma-ray lines from SN1987A
โ Scribed by B.J. Teegarden
- Publisher
- Elsevier Science
- Year
- 1991
- Tongue
- English
- Weight
- 820 KB
- Volume
- 11
- Category
- Article
- ISSN
- 0273-1177
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