Cultural advice

The Australian National University acknowledges, celebrates and pays our respects to the Ngunnawal and Ngambri people of the Canberra region and to all First Nations Australians on whose traditional lands we meet and work, and whose cultures are among the oldest continuing cultures in human history.

Aboriginal and Torres Strait Islander peoples are advised that ANU Library collections may include images, names, voices, and other representations of deceased persons.

Material in the collection may contain terms, language or views that reflect the period in which the item was created and may be considered inappropriate today.

The lithium isotopic ratio in very metal-poor stars

Date

Authors

Lind, Karin

Melendez, Jorge

Asplund, Martin

Collet, Remo

Magic, Zazralt

Publisher

Springer

Abstract

Context. Un-evolved, very metal-poor stars are the most important tracers of the cosmic abundance of lithium in the early universe. Combining the standard Big Bang nucleosynthesis model with Galactic production through cosmic ray spallation, these stars a

Keywords

Keywords: Line: formation; Line: Profiles; Primordial nucleosynthesis; Stars: abundances; Stars: Population II; Techniques: spectroscopic; Calcium; Hydrogen bonds; Isotopes; Lithium; Nucleosynthesis; Sodium; Three dimensional; Three dimensional computer graphics; S Line: formation; Line: profiles; Primordial nucleosynthesis; Stars: abundances; Stars: Population II; Techniques: spectroscopic

URI

http://hdl.handle.net/1885/72987

Collections

ANU Research Publications

Source

Astronomy and Astrophysics

Type

Journal article

Access Statement

Open Access

DOI

10.1051/0004-6361/201321406

Downloads

File

Description

01_Lind_The_lithium_isotopic_ratio_in_2013.pdf (1.37 MB)

abcd