ReP USP - Resultado da busca

Artigo de periodico
High-resolution abundance analysis of four red giants in the globular cluster NGC 6558 (2018)
Barbuy, Beatriz Leonor Silveira; Muniz, L; Ortolani, S; Ernandes, H; Dias, B; Saviane, I; Kerber, L; Bica, E; Pérez-Villegas, A; Rossi, L; Held, E.V
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, CENTRO GALÁCTICO, AGLOMERADOS (GALÁXIA), GALÁXIA (VIA LÁCTEA)
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ABNT
BARBUY, Beatriz Leonor Silveira et al. High-resolution abundance analysis of four red giants in the globular cluster NGC 6558. Astronomy & Astrophysics, v. 619, p. A178, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201833953. Acesso em: 07 nov. 2024.
APA
Barbuy, B. L. S., Muniz, L., Ortolani, S., Ernandes, H., Dias, B., Saviane, I., et al. (2018). High-resolution abundance analysis of four red giants in the globular cluster NGC 6558. Astronomy & Astrophysics, 619, A178. doi:10.1051/0004-6361/201833953
NLM
Barbuy BLS, Muniz L, Ortolani S, Ernandes H, Dias B, Saviane I, Kerber L, Bica E, Pérez-Villegas A, Rossi L, Held EV. High-resolution abundance analysis of four red giants in the globular cluster NGC 6558 [Internet]. Astronomy & Astrophysics. 2018 ; 619 A178.[citado 2024 nov. 07 ] Available from: https://doi.org/10.1051/0004-6361/201833953
Vancouver
Barbuy BLS, Muniz L, Ortolani S, Ernandes H, Dias B, Saviane I, Kerber L, Bica E, Pérez-Villegas A, Rossi L, Held EV. High-resolution abundance analysis of four red giants in the globular cluster NGC 6558 [Internet]. Astronomy & Astrophysics. 2018 ; 619 A178.[citado 2024 nov. 07 ] Available from: https://doi.org/10.1051/0004-6361/201833953
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: 07 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. 07 ] 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. 07 ] 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: 07 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. 07 ] 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. 07 ] 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
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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: 07 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. 07 ] 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. 07 ] 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: 07 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. 07 ]
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. 07 ]
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: 07 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. 07 ]
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. 07 ]
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: 07 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. 07 ]
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. 07 ]
Artigo de periodico
Age and metallicity of star clusters in the Small Magellanic Cloud from integrated spectroscopy (2010)
Dias, B; Coelho, P; Barbuy, Beatriz Leonor Silveira; Kerber, L; Idiart, Thais Eunice Pires
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: NUVENS DE MAGALHÃES, GALÁXIAS, ESTRELAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
DIAS, B et al. Age and metallicity of star clusters in the Small Magellanic Cloud from integrated spectroscopy. Astronomy & Astrophysics, v. 520, p. A85/1-A85/17, 2010Tradução . . Disponível em: https://doi.org/10.1017/s174392131000308x. Acesso em: 07 nov. 2024.
APA
Dias, B., Coelho, P., Barbuy, B. L. S., Kerber, L., & Idiart, T. E. P. (2010). Age and metallicity of star clusters in the Small Magellanic Cloud from integrated spectroscopy. Astronomy & Astrophysics, 520, A85/1-A85/17. doi:10.1017/s174392131000308x
NLM
Dias B, Coelho P, Barbuy BLS, Kerber L, Idiart TEP. Age and metallicity of star clusters in the Small Magellanic Cloud from integrated spectroscopy [Internet]. Astronomy & Astrophysics. 2010 ; 520 A85/1-A85/17.[citado 2024 nov. 07 ] Available from: https://doi.org/10.1017/s174392131000308x
Vancouver
Dias B, Coelho P, Barbuy BLS, Kerber L, Idiart TEP. Age and metallicity of star clusters in the Small Magellanic Cloud from integrated spectroscopy [Internet]. Astronomy & Astrophysics. 2010 ; 520 A85/1-A85/17.[citado 2024 nov. 07 ] Available from: https://doi.org/10.1017/s174392131000308x

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