HST-STIS abundances in the uranium-rich very metal poor star CS 31082-001 (2010)
- Authors:
- Autor USP: BARBUY, BEATRIZ LEONOR SILVEIRA - IAG
- Unidade: IAG
- Subjects: ESTRELAS; RADIAÇÃO ULTRAVIOLETA; URÂNIO
- Language: Inglês
- Imprenta:
- Publisher: Cambridge University Press
- Publisher place: Cambridge
- Date published: 2010
- Source:
- Conference titles: IAU Symposium
-
ABNT
BARBUY, Beatriz Leonor Silveira et al. HST-STIS abundances in the uranium-rich very metal poor star CS 31082-001. 2010, Anais.. Cambridge: Cambridge University Press, 2010. . Acesso em: 25 fev. 2026. -
APA
Barbuy, B. L. S., Spite, M., Hill, V., & Sneden, C. (2010). HST-STIS abundances in the uranium-rich very metal poor star CS 31082-001. In Chemical abundances in the Universe : connecting first stars to planets. Proceedings. Cambridge: Cambridge University Press. -
NLM
Barbuy BLS, Spite M, Hill V, Sneden C. HST-STIS abundances in the uranium-rich very metal poor star CS 31082-001. Chemical abundances in the Universe : connecting first stars to planets. Proceedings. 2010 ;[citado 2026 fev. 25 ] -
Vancouver
Barbuy BLS, Spite M, Hill V, Sneden C. HST-STIS abundances in the uranium-rich very metal poor star CS 31082-001. Chemical abundances in the Universe : connecting first stars to planets. Proceedings. 2010 ;[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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