The ideal stars for exploration of early-epoch 'ANTIPOT.7 LI' abundances (1999)
- Authors:
- Autor USP: ROSSI, SILVIA CRISTINA FERNANDES - IAG
- Unidade: IAG
- Subjects: ASTRONOMIA; MEIO INTERESTELAR
- Language: Inglês
- Imprenta:
- Source:
- Conference titles: International Astronomical Union
-
ABNT
ROSSI, Silvia Cristina Fernandes e BEERS, T. C. The ideal stars for exploration of early-epoch 'ANTIPOT.7 LI' abundances. 1999, Anais.. São Paulo: IAG-USP, 1999. . Acesso em: 15 fev. 2026. -
APA
Rossi, S. C. F., & Beers, T. C. (1999). The ideal stars for exploration of early-epoch 'ANTIPOT.7 LI' abundances. In The light elements and their evolution : program and abstracts. São Paulo: IAG-USP. -
NLM
Rossi SCF, Beers TC. The ideal stars for exploration of early-epoch 'ANTIPOT.7 LI' abundances. The light elements and their evolution : program and abstracts. 1999 ;[citado 2026 fev. 15 ] -
Vancouver
Rossi SCF, Beers TC. The ideal stars for exploration of early-epoch 'ANTIPOT.7 LI' abundances. The light elements and their evolution : program and abstracts. 1999 ;[citado 2026 fev. 15 ] - Broadband UBVRcIc photometry of horizontal-branch and metal-poor candidates from the HK and Hamburg/ESO surveys. I.
- Metal-poor stars observed with the Magellan Telescope.: II. Discovery of four stars with [Fe/H] <= -3,5
- The Hamburg/ESO R-process enhanced star survey (HERES): II. Spectroscopic analysis of the survey sample
- Metal abundance estimates for F- and G-type stars from Edinburgh-cape blue object survey
- Estimativas de precisão de temperaturas efetivas estelares e avermelhamento interestelar utilizando o índice de linha de Balmer baseado em espectroscopia de média resolução
- Bright metal-poor stars from the Hamburg/ESO survey: I. Selection and follow-up observations from 329 fields
- The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey
- Elemental abundances and classification of carbon-enhanced metal-poor stars
- Additional emission-line candidates from the hk survey
- Spectroscopic validation of low-metallicity stars from RAVE
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