Abundances in very metal-poor stars (1999)
- Authors:
- Autor USP: BARBUY, BEATRIZ LEONOR SILVEIRA - IAG
- Unidade: IAG
- Subjects: ASTRONOMIA; ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Source:
- Título: Astrophysics and Space Science
- Volume/Número/Paginação/Ano: v. 265, n. 1-4, p. 141-144, 1999
-
ABNT
SPITE, M. et al. Abundances in very metal-poor stars. Astrophysics and Space Science, v. 265, n. 1-4, p. 141-144, 1999Tradução . . Acesso em: 25 fev. 2026. -
APA
Spite, M., Spite, F., Cayrel, R., Hill, V., Nordströn, B., Barbuy, B. L. S., et al. (1999). Abundances in very metal-poor stars. Astrophysics and Space Science, 265( 1-4), 141-144. -
NLM
Spite M, Spite F, Cayrel R, Hill V, Nordströn B, Barbuy BLS, Beers T, Nissen PE. Abundances in very metal-poor stars. Astrophysics and Space Science. 1999 ; 265( 1-4): 141-144.[citado 2026 fev. 25 ] -
Vancouver
Spite M, Spite F, Cayrel R, Hill V, Nordströn B, Barbuy BLS, Beers T, Nissen PE. Abundances in very metal-poor stars. Astrophysics and Space Science. 1999 ; 265( 1-4): 141-144.[citado 2026 fev. 25 ] - Ages of the bulge globular clusters NGC 6522 and NGC 6626 (M28) from HST proper-motion-cleaned color–magnitude diagrams*
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