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Filtros : "Endl, M" Removido: "França" Limpar

Filtros

Artigo de periodico
Constraining teh evolutionofstellar rotation using solar twins (2019)
Lorenzo-Oliveira, Diego; Moreno, Jorge Luiz Meléndez; Lichon, S. J; Chanamé, J; Endl, M; Moreno, Jorge Luis Meléndez; Lambert, D. L.
Fonte: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Assuntos: ASTROFISICA ESTELAR, SOL
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
LORENZO-OLIVEIRA, Diego et al. Constraining teh evolutionofstellar rotation using solar twins. Monthly Notices of the Royal Astronomical Society, v. 490, p. 2448-2457, 2019Tradução . . Disponível em: https://academic.oup.com/mnras/article/490/2/2448/5583050. Acesso em: 26 out. 2025.
APA
Lorenzo-Oliveira, D., Moreno, J. L. M., Lichon, S. J., Chanamé, J., Endl, M., Moreno, J. L. M., & Lambert, D. L. (2019). Constraining teh evolutionofstellar rotation using solar twins. Monthly Notices of the Royal Astronomical Society, 490, 2448-2457. doi:10.1093/mnras/slz034
NLM
Lorenzo-Oliveira D, Moreno JLM, Lichon SJ, Chanamé J, Endl M, Moreno JLM, Lambert DL. Constraining teh evolutionofstellar rotation using solar twins [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 2448-2457.[citado 2025 out. 26 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
Vancouver
Lorenzo-Oliveira D, Moreno JLM, Lichon SJ, Chanamé J, Endl M, Moreno JLM, Lambert DL. Constraining teh evolutionofstellar rotation using solar twins [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 2448-2457.[citado 2025 out. 26 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
Artigo de periodico
The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs (2019)
Ramirez; Khanal, S.; Lichon, S. J; Chanamé, J; Endl, M; Moreno, Jorge Luis Meléndez; Lambert, D. L.
Fonte: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Assuntos: ABUNDÂNCIA ESTELAR, ESTRELAS BINARIAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
RAMIREZ, et al. The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs. Monthly Notices of the Royal Astronomical Society, v. 490, p. 2448-2457, 2019Tradução . . Disponível em: https://academic.oup.com/mnras/article/490/2/2448/5583050. Acesso em: 26 out. 2025.
APA
Ramirez,, Khanal, S., Lichon, S. J., Chanamé, J., Endl, M., Moreno, J. L. M., & Lambert, D. L. (2019). The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs. Monthly Notices of the Royal Astronomical Society, 490, 2448-2457. doi:10.1093/mnras/sty104
NLM
Ramirez, Khanal S, Lichon SJ, Chanamé J, Endl M, Moreno JLM, Lambert DL. The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 2448-2457.[citado 2025 out. 26 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
Vancouver
Ramirez, Khanal S, Lichon SJ, Chanamé J, Endl M, Moreno JLM, Lambert DL. The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 2448-2457.[citado 2025 out. 26 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050

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