Production and evolution of Li, Be, and B isotopes in the Galaxy

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Volume 542 (June 2012)

A&A, 542 (2012) A67

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Table 2

Yields of Li (in M_⊙) from low-mass sources.

	Inferred from	Calculated
	this work^a	in literature (Ref.)

Novae	10^-9	10^-10 (1)
AGB (2–6 M_⊙)	1.5 × 10^-7	<3 × 10^-8 (2, 3)
AGB (2–4 M_⊙)	2 × 10^-7	<5 × 10^-9 (2)
RG (1–2 M_⊙)	1 × 10^-7	<10^-8 (3)

Notes.

^(a)

Under the assumption that each class of sources produces 50% of solar Li (the remaining coming from SBBN+GCR+ ν-nucleosynthesis in CCSN).

References. (1): Hernanz et al. (1996), (2): Ventura and d’Antona, yields presented in Romano et al. (2001); and (3): Travaglio et al. (2001).

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