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

N. Prantzos

doi:10.1051/0004-6361/201219043

Home

All issues

Volume 542 (June 2012)

A&A, 542 (2012) A67

Full HTML

Free Access

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).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.