High-resolution spectroscopy of giant stars in the open clusters IC 4651 and IC 4725 (2016)
- Authors:
- Autor USP: ROSSI, SILVIA CRISTINA FERNANDES - IAG
- Unidade: IAG
- Subjects: ASTROFÍSICA ESTELAR; ESPECTROSCOPIA
- Language: Inglês
- Imprenta:
- Source:
- Título: ASOS -12
- Conference titles: International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas
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ABNT
SANTRICH, Orlando J. Katime e ROSSI, Silvia Cristina Fernandes e ALVES-BRITO, A. High-resolution spectroscopy of giant stars in the open clusters IC 4651 and IC 4725. 2016, Anais.. São Paulo: IAG/USP, 2016. . Acesso em: 01 mar. 2026. -
APA
Santrich, O. J. K., Rossi, S. C. F., & Alves-Brito, A. (2016). High-resolution spectroscopy of giant stars in the open clusters IC 4651 and IC 4725. In ASOS -12. São Paulo: IAG/USP. -
NLM
Santrich OJK, Rossi SCF, Alves-Brito A. High-resolution spectroscopy of giant stars in the open clusters IC 4651 and IC 4725. ASOS -12. 2016 ;[citado 2026 mar. 01 ] -
Vancouver
Santrich OJK, Rossi SCF, Alves-Brito A. High-resolution spectroscopy of giant stars in the open clusters IC 4651 and IC 4725. ASOS -12. 2016 ;[citado 2026 mar. 01 ] - 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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