Refined estimates of carbon abundances for carbon-enhanced stars (2008)
- Authors:
- Autor USP: ROSSI, SILVIA CRISTINA FERNANDES - IAG
- Unidade: IAG
- Subjects: ESTRELAS; CARBONO
- Language: Inglês
- Imprenta:
- Publisher: Scuola Internazionale Superiore di Studi Avanzati
- Publisher place: Trieste
- Date published: 2008
- Source:
- Título: Proceedings of Science: NIC X
- ISSN: 1824-8039
- Conference titles: Symposium on Nuclei in the Cosmos
-
ABNT
ROSSI, Silvia Cristina Fernandes et al. Refined estimates of carbon abundances for carbon-enhanced stars. 2008, Anais.. Trieste: Scuola Internazionale Superiore di Studi Avanzati, 2008. . Acesso em: 05 mar. 2026. -
APA
Rossi, S. C. F., Placco, V. M., Beers, T. C., Kennedy, C. R., & Marsteller, B. (2008). Refined estimates of carbon abundances for carbon-enhanced stars. In Proceedings of Science: NIC X. Trieste: Scuola Internazionale Superiore di Studi Avanzati. -
NLM
Rossi SCF, Placco VM, Beers TC, Kennedy CR, Marsteller B. Refined estimates of carbon abundances for carbon-enhanced stars. Proceedings of Science: NIC X. 2008 ;[citado 2026 mar. 05 ] -
Vancouver
Rossi SCF, Placco VM, Beers TC, Kennedy CR, Marsteller B. Refined estimates of carbon abundances for carbon-enhanced stars. Proceedings of Science: NIC X. 2008 ;[citado 2026 mar. 05 ] - 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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