First satrs IV. CS 29497-030: evidence for operation of the s-process at very low metallicity (2004)
- Authors:
- Autor USP: BARBUY, BEATRIZ LEONOR SILVEIRA - IAG
- Unidade: IAG
- Assunto: ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Source:
- Título: Astronomy and Astrophysics
- ISSN: 0004-6361
- Volume/Número/Paginação/Ano: v. 413, p.1073-1085, 2004
-
ABNT
SIVARANI, T et al. First satrs IV. CS 29497-030: evidence for operation of the s-process at very low metallicity. Astronomy and Astrophysics, v. 413, p. 1073-1085, 2004Tradução . . Acesso em: 17 nov. 2024. -
APA
Sivarani, T., Bonifacio, P., Molaro, P., Cayrel, R., Spite, M., Spite, F., et al. (2004). First satrs IV. CS 29497-030: evidence for operation of the s-process at very low metallicity. Astronomy and Astrophysics, 413, 1073-1085. -
NLM
Sivarani T, Bonifacio P, Molaro P, Cayrel R, Spite M, Spite F, Plez B, Andersen J, Barbuy BLS, Beers TC, Depagne E, Hill V, François P, Nordström B, Primas F. First satrs IV. CS 29497-030: evidence for operation of the s-process at very low metallicity. Astronomy and Astrophysics. 2004 ; 413 1073-1085.[citado 2024 nov. 17 ] -
Vancouver
Sivarani T, Bonifacio P, Molaro P, Cayrel R, Spite M, Spite F, Plez B, Andersen J, Barbuy BLS, Beers TC, Depagne E, Hill V, François P, Nordström B, Primas F. First satrs IV. CS 29497-030: evidence for operation of the s-process at very low metallicity. Astronomy and Astrophysics. 2004 ; 413 1073-1085.[citado 2024 nov. 17 ] - VLT-UVES Spectroscopy of the subgiant I-24 of the bulge globular cluster NGC 6528 in baade´s window
- Mapping out the interstellar extinction in the central 10 degrees of the galaxy with 2MASS
- Aglomerados globulares das nuvens de Magalhães: idade e metalicidades
- A new approach to derive ['alfa'/Fe] for integrated stellar populations
- Metal-poor globular clusters of the galactic bulge
- Physical parameters of intermediate-age LMC clusters from modelling of HST CMDs
- The distance and space distribution of bulge globular clusters
- Halo chemistry and first stars. The chemical composition of the matter in the early Galaxy, from C to Mg
- Vista Variables in the Via Lactea (VVV)
- Identificação das linhas espectrais da estrela ultra pobre em metais CS 31082-001
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas