ReP USP - Resultado da busca

Artigo de periodico
SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients (2016)
Dias, B; Kerber, L; Barbuy, Beatriz Leonor Silveira; Bica, E; Ortolani, S
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: GALÁXIAS, NUVENS DE MAGALHÃES
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
DIAS, B et al. SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients. Astronomy & Astrophysics, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527558. Acesso em: 04 nov. 2024.
APA
Dias, B., Kerber, L., Barbuy, B. L. S., Bica, E., & Ortolani, S. (2016). SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients. Astronomy & Astrophysics. doi:10.1051/0004-6361/201527558
NLM
Dias B, Kerber L, Barbuy BLS, Bica E, Ortolani S. SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients [Internet]. Astronomy & Astrophysics. 2016 ;[citado 2024 nov. 04 ] Available from: https://doi.org/10.1051/0004-6361/201527558
Vancouver
Dias B, Kerber L, Barbuy BLS, Bica E, Ortolani S. SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients [Internet]. Astronomy & Astrophysics. 2016 ;[citado 2024 nov. 04 ] Available from: https://doi.org/10.1051/0004-6361/201527558
Artigo de periodico
SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients (2016)
Dias, B; Kerber, L; Barbuy, Beatriz Leonor Silveira; Bica, E; Ortolani, S
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: GALÁXIAS, ESTRELAS, NUVENS DE MAGALHÃES
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
DIAS, B et al. SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients. Astronomy & Astrophysics, v. 591, p. A11/1-A11/16, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527558. Acesso em: 04 nov. 2024.
APA
Dias, B., Kerber, L., Barbuy, B. L. S., Bica, E., & Ortolani, S. (2016). SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients. Astronomy & Astrophysics, 591, A11/1-A11/16. doi:10.1051/0004-6361/201527558
NLM
Dias B, Kerber L, Barbuy BLS, Bica E, Ortolani S. SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients [Internet]. Astronomy & Astrophysics. 2016 ; 591 A11/1-A11/16.[citado 2024 nov. 04 ] Available from: https://doi.org/10.1051/0004-6361/201527558
Vancouver
Dias B, Kerber L, Barbuy BLS, Bica E, Ortolani S. SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients [Internet]. Astronomy & Astrophysics. 2016 ; 591 A11/1-A11/16.[citado 2024 nov. 04 ] Available from: https://doi.org/10.1051/0004-6361/201527558
Artigo de periodico
Bridge over troubled gas: clusters and associations under the SMC and LMC tidal stresses (2015)
Bica, E; Santiago, B; Bonatto, C; Garcia-Dias, R; Kerber, L; Dias, B; Barbuy, Beatriz Leonor Silveira; Balbinot, E
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: NUVENS DE MAGALHÃES, AGLOMERADOS DE GALÁXIAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
BICA, E et al. Bridge over troubled gas: clusters and associations under the SMC and LMC tidal stresses. Monthly Notices of the Royal Astronomical Society, v. 453, p. 3190-3102, 2015Tradução . . Disponível em: https://doi.org/10.1093/mnras/stv1720. Acesso em: 04 nov. 2024.
APA
Bica, E., Santiago, B., Bonatto, C., Garcia-Dias, R., Kerber, L., Dias, B., et al. (2015). Bridge over troubled gas: clusters and associations under the SMC and LMC tidal stresses. Monthly Notices of the Royal Astronomical Society, 453, 3190-3102. doi:10.1093/mnras/stv1720
NLM
Bica E, Santiago B, Bonatto C, Garcia-Dias R, Kerber L, Dias B, Barbuy BLS, Balbinot E. Bridge over troubled gas: clusters and associations under the SMC and LMC tidal stresses [Internet]. Monthly Notices of the Royal Astronomical Society. 2015 ; 453 3190-3102.[citado 2024 nov. 04 ] Available from: https://doi.org/10.1093/mnras/stv1720
Vancouver
Bica E, Santiago B, Bonatto C, Garcia-Dias R, Kerber L, Dias B, Barbuy BLS, Balbinot E. Bridge over troubled gas: clusters and associations under the SMC and LMC tidal stresses [Internet]. Monthly Notices of the Royal Astronomical Society. 2015 ; 453 3190-3102.[citado 2024 nov. 04 ] Available from: https://doi.org/10.1093/mnras/stv1720
Trabalho de evento-resumo
Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling (2014)
Dias, B; Kerber, L; Barbuy, Beatriz Leonor Silveira; Santiago, B; Ortoloni, S; Balbinot, E
Source: ASP Conference Series. Conference titles: Fifty Years of Wide Field Studies in the Southern Hemisphere: Resolved Stellar Populations of the Galactic Bulge and the Magellanic Clouds. Unidade: IAG
Subjects: POPULAÇÕES ESTELARES, NUVENS DE MAGALHÃES
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
DIAS, B et al. Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling. 2014, Anais.. San Francisco: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, 2014. p. 338. . Acesso em: 04 nov. 2024.
APA
Dias, B., Kerber, L., Barbuy, B. L. S., Santiago, B., Ortoloni, S., & Balbinot, E. (2014). Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling. In ASP Conference Series (Vol. 491, p. 338). San Francisco: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo.
NLM
Dias B, Kerber L, Barbuy BLS, Santiago B, Ortoloni S, Balbinot E. Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling. ASP Conference Series. 2014 ; 491 338.[citado 2024 nov. 04 ]
Vancouver
Dias B, Kerber L, Barbuy BLS, Santiago B, Ortoloni S, Balbinot E. Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling. ASP Conference Series. 2014 ; 491 338.[citado 2024 nov. 04 ]
Trabalho de evento-resumo periodico
Parameters for SMC clusters from CMD modeling (2014)
Dias, B; Kerber, L; Barbuy, Beatriz Leonor Silveira; Santiago, B; Ortolani, S; Balbinot, E
Source: Revista Mexicana de Astronomía y Astrofísica. Serie de Conferencias. Conference titles: Latin American Regional IAU Meeting. Unidade: IAG
Assunto: NUVENS DE MAGALHÃES
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
DIAS, B et al. Parameters for SMC clusters from CMD modeling. Revista Mexicana de Astronomía y Astrofísica. Serie de Conferencias. México: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. . Acesso em: 04 nov. 2024. , 2014
APA
Dias, B., Kerber, L., Barbuy, B. L. S., Santiago, B., Ortolani, S., & Balbinot, E. (2014). Parameters for SMC clusters from CMD modeling. Revista Mexicana de Astronomía y Astrofísica. Serie de Conferencias. México: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo.
NLM
Dias B, Kerber L, Barbuy BLS, Santiago B, Ortolani S, Balbinot E. Parameters for SMC clusters from CMD modeling. Revista Mexicana de Astronomía y Astrofísica. Serie de Conferencias. 2014 ; 44 153.[citado 2024 nov. 04 ]
Vancouver
Dias B, Kerber L, Barbuy BLS, Santiago B, Ortolani S, Balbinot E. Parameters for SMC clusters from CMD modeling. Revista Mexicana de Astronomía y Astrofísica. Serie de Conferencias. 2014 ; 44 153.[citado 2024 nov. 04 ]
Trabalho de evento-resumo
Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling (2013)
Dias, B; Kerber, L; Barbuy, Beatriz Leonor Silveira; Santiago, B; Ortolani, S; Balbinot, E
Source: LARIM 2013: Abstract Book. Conference titles: Latin American Regional IAU Meeting. Unidade: IAG
Subjects: NUVENS DE MAGALHÃES, ESTRELAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
DIAS, B et al. Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling. 2013, Anais.. Paris: International Astronomical Union, 2013. . Acesso em: 04 nov. 2024.
APA
Dias, B., Kerber, L., Barbuy, B. L. S., Santiago, B., Ortolani, S., & Balbinot, E. (2013). Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling. In LARIM 2013: Abstract Book. Paris: International Astronomical Union.
NLM
Dias B, Kerber L, Barbuy BLS, Santiago B, Ortolani S, Balbinot E. Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling. LARIM 2013: Abstract Book. 2013 ;[citado 2024 nov. 04 ]
Vancouver
Dias B, Kerber L, Barbuy BLS, Santiago B, Ortolani S, Balbinot E. Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling. LARIM 2013: Abstract Book. 2013 ;[citado 2024 nov. 04 ]

USP Schools

ReP

Filtros

Authors

Non normalized affiliation