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Filtros : "Dias, W S" Removido: "ASTRONOMIA" Limpar

Filtros

Artigo de periodico
Models for the 3D axisymmetric gravitational potential of the Milky Way galaxy: a detailed modelling of the Galactic disk (2016)
Barros, D. A; Lépine, Jacques Raymond Daniel; Dias, W S
Source: Astronomy & Astronomy. Unidade: IAG
Subjects: ESTRUTURA DA GALÁXIA, GALÁXIA (VIA LÁCTEA)
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
BARROS, D. A e LÉPINE, Jacques Raymond Daniel e DIAS, W S. Models for the 3D axisymmetric gravitational potential of the Milky Way galaxy: a detailed modelling of the Galactic disk. Astronomy & Astronomy, v. 593, n. 108, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527535. Acesso em: 16 out. 2024.
APA
Barros, D. A., Lépine, J. R. D., & Dias, W. S. (2016). Models for the 3D axisymmetric gravitational potential of the Milky Way galaxy: a detailed modelling of the Galactic disk. Astronomy & Astronomy, 593( 108). doi:10.1051/0004-6361/201527535
NLM
Barros DA, Lépine JRD, Dias WS. Models for the 3D axisymmetric gravitational potential of the Milky Way galaxy: a detailed modelling of the Galactic disk [Internet]. Astronomy & Astronomy. 2016 ;593( 108):[citado 2024 out. 16 ] Available from: https://doi.org/10.1051/0004-6361/201527535
Vancouver
Barros DA, Lépine JRD, Dias WS. Models for the 3D axisymmetric gravitational potential of the Milky Way galaxy: a detailed modelling of the Galactic disk [Internet]. Astronomy & Astronomy. 2016 ;593( 108):[citado 2024 out. 16 ] Available from: https://doi.org/10.1051/0004-6361/201527535
Artigo de periodico
Proper motions of the optically visible open clusters based on the UCAC4 catalog (2014)
Dias, W S; Monteiro, H.; Caetano, T. C; Lépine, Jacques Raymond Daniel; Assafin, M; Oliveira, A. F.
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: AGLOMERADOS DE GALÁXIAS, ESTRELAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
DIAS, W S et al. Proper motions of the optically visible open clusters based on the UCAC4 catalog. Astronomy & Astrophysics, v. 564, p. A79/1-A79/8, 2014Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201323226. Acesso em: 16 out. 2024.
APA
Dias, W. S., Monteiro, H., Caetano, T. C., Lépine, J. R. D., Assafin, M., & Oliveira, A. F. (2014). Proper motions of the optically visible open clusters based on the UCAC4 catalog. Astronomy & Astrophysics, 564, A79/1-A79/8. doi:10.1051/0004-6361/201323226
NLM
Dias WS, Monteiro H, Caetano TC, Lépine JRD, Assafin M, Oliveira AF. Proper motions of the optically visible open clusters based on the UCAC4 catalog [Internet]. Astronomy & Astrophysics. 2014 ; 564 A79/1-A79/8.[citado 2024 out. 16 ] Available from: https://doi.org/10.1051/0004-6361/201323226
Vancouver
Dias WS, Monteiro H, Caetano TC, Lépine JRD, Assafin M, Oliveira AF. Proper motions of the optically visible open clusters based on the UCAC4 catalog [Internet]. Astronomy & Astrophysics. 2014 ; 564 A79/1-A79/8.[citado 2024 out. 16 ] Available from: https://doi.org/10.1051/0004-6361/201323226

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