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Artigo de periodico
FORS2/VLT survey of Milky Way globular clusters: I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8 (2015)
Dias, B; Barbuy, Beatriz Leonor Silveira; Saviane, I; Held, E. V; Costa, G. S. da; Ortolani, S; Vásquez, S; Gullieuszik, M; Katz, D
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR, CINEMÁTICA, DINÂMICA, POPULAÇÕES ESTELARES, GALÁXIA (VIA LÁCTEA)
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
DIAS, B et al. FORS2/VLT survey of Milky Way globular clusters: I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8. Astronomy & Astrophysics, v. 573, p. A13/1-A13/23, 2015Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201423996. Acesso em: 07 jul. 2024.
APA
Dias, B., Barbuy, B. L. S., Saviane, I., Held, E. V., Costa, G. S. da, Ortolani, S., et al. (2015). FORS2/VLT survey of Milky Way globular clusters: I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8. Astronomy & Astrophysics, 573, A13/1-A13/23. doi:10.1051/0004-6361/201423996
NLM
Dias B, Barbuy BLS, Saviane I, Held EV, Costa GS da, Ortolani S, Vásquez S, Gullieuszik M, Katz D. FORS2/VLT survey of Milky Way globular clusters: I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8 [Internet]. Astronomy & Astrophysics. 2015 ; 573 A13/1-A13/23.[citado 2024 jul. 07 ] Available from: https://doi.org/10.1051/0004-6361/201423996
Vancouver
Dias B, Barbuy BLS, Saviane I, Held EV, Costa GS da, Ortolani S, Vásquez S, Gullieuszik M, Katz D. FORS2/VLT survey of Milky Way globular clusters: I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8 [Internet]. Astronomy & Astrophysics. 2015 ; 573 A13/1-A13/23.[citado 2024 jul. 07 ] Available from: https://doi.org/10.1051/0004-6361/201423996
Artigo de periodico
2.5D global-disk oscillation models of the Be shell star 'dzeta' Tauri: I. Spectroscopic and polarimetric analysis (2015)
Escolano, C; Carciofi, Alex Cavaliéri; Okazaki, A. T; Rivinius, T; Baade, D; Štefl,S
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: MÉTODOS NUMÉRICOS, TRANSFERÊNCIA RADIATIVA, ESTRELAS, CINEMÁTICA, DINÂMICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
ESCOLANO, C et al. 2.5D global-disk oscillation models of the Be shell star 'dzeta' Tauri: I. Spectroscopic and polarimetric analysis. Astronomy & Astrophysics, v. 576, p. A112/1-A112/15, 2015Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201425446. Acesso em: 07 jul. 2024.
APA
Escolano, C., Carciofi, A. C., Okazaki, A. T., Rivinius, T., Baade, D., & Štefl, S. (2015). 2.5D global-disk oscillation models of the Be shell star 'dzeta' Tauri: I. Spectroscopic and polarimetric analysis. Astronomy & Astrophysics, 576, A112/1-A112/15. doi:10.1051/0004-6361/201425446
NLM
Escolano C, Carciofi AC, Okazaki AT, Rivinius T, Baade D, Štefl S. 2.5D global-disk oscillation models of the Be shell star 'dzeta' Tauri: I. Spectroscopic and polarimetric analysis [Internet]. Astronomy & Astrophysics. 2015 ; 576 A112/1-A112/15.[citado 2024 jul. 07 ] Available from: https://doi.org/10.1051/0004-6361/201425446
Vancouver
Escolano C, Carciofi AC, Okazaki AT, Rivinius T, Baade D, Štefl S. 2.5D global-disk oscillation models of the Be shell star 'dzeta' Tauri: I. Spectroscopic and polarimetric analysis [Internet]. Astronomy & Astrophysics. 2015 ; 576 A112/1-A112/15.[citado 2024 jul. 07 ] Available from: https://doi.org/10.1051/0004-6361/201425446
Artigo de periodico
Formation and evolution of the two 4/3 resonant giants planets in HD 200964 (2015)
Tadeu dos Santos, M; Correa-Otto, J. A; Michtchenko, Tatiana Alexandrovna; Ferraz-Mello, Sylvio
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: PLANETAS (FORMAÇÃO), SATÉLITES (FORMAÇÃO), DINÂMICA, MECÂNICA CELESTE
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
TADEU DOS SANTOS, M et al. Formation and evolution of the two 4/3 resonant giants planets in HD 200964. Astronomy & Astrophysics, v. 573, p. A94/1-A94/15, 2015Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201424820. Acesso em: 07 jul. 2024.
APA
Tadeu dos Santos, M., Correa-Otto, J. A., Michtchenko, T. A., & Ferraz-Mello, S. (2015). Formation and evolution of the two 4/3 resonant giants planets in HD 200964. Astronomy & Astrophysics, 573, A94/1-A94/15. doi:10.1051/0004-6361/201424820
NLM
Tadeu dos Santos M, Correa-Otto JA, Michtchenko TA, Ferraz-Mello S. Formation and evolution of the two 4/3 resonant giants planets in HD 200964 [Internet]. Astronomy & Astrophysics. 2015 ; 573 A94/1-A94/15.[citado 2024 jul. 07 ] Available from: https://doi.org/10.1051/0004-6361/201424820
Vancouver
Tadeu dos Santos M, Correa-Otto JA, Michtchenko TA, Ferraz-Mello S. Formation and evolution of the two 4/3 resonant giants planets in HD 200964 [Internet]. Astronomy & Astrophysics. 2015 ; 573 A94/1-A94/15.[citado 2024 jul. 07 ] Available from: https://doi.org/10.1051/0004-6361/201424820

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