ReP USP - Resultado da busca

Artigo de periodico
FORS2/VLT survey of Milky Way globular clusters: II. Fe and Mg abundances of 51 Milky Way globular clusters on a homogeneous scale (2016)
Dias, B; Barbuy, Beatriz Leonor Silveira; Saviane, I; Held, E. V; Da Costa, G. S; Ortolani, S; Gullieuszik, M; Vásquez, S
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, DINÂMICA, CINEMÁTICA, POPULAÇÕES ESTELARES, FORMAÇÃO E EVOLUÇÃO DA GALÁXIA
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ABNT
DIAS, B et al. FORS2/VLT survey of Milky Way globular clusters: II. Fe and Mg abundances of 51 Milky Way globular clusters on a homogeneous scale. Astronomy & Astrophysics, v. 590, p. A9/1-A9/15, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201526765. Acesso em: 11 ago. 2024.
APA
Dias, B., Barbuy, B. L. S., Saviane, I., Held, E. V., Da Costa, G. S., Ortolani, S., et al. (2016). FORS2/VLT survey of Milky Way globular clusters: II. Fe and Mg abundances of 51 Milky Way globular clusters on a homogeneous scale. Astronomy & Astrophysics, 590, A9/1-A9/15. doi:10.1051/0004-6361/201526765
NLM
Dias B, Barbuy BLS, Saviane I, Held EV, Da Costa GS, Ortolani S, Gullieuszik M, Vásquez S. FORS2/VLT survey of Milky Way globular clusters: II. Fe and Mg abundances of 51 Milky Way globular clusters on a homogeneous scale [Internet]. Astronomy & Astrophysics. 2016 ; 590 A9/1-A9/15.[citado 2024 ago. 11 ] Available from: https://doi.org/10.1051/0004-6361/201526765
Vancouver
Dias B, Barbuy BLS, Saviane I, Held EV, Da Costa GS, Ortolani S, Gullieuszik M, Vásquez S. FORS2/VLT survey of Milky Way globular clusters: II. Fe and Mg abundances of 51 Milky Way globular clusters on a homogeneous scale [Internet]. Astronomy & Astrophysics. 2016 ; 590 A9/1-A9/15.[citado 2024 ago. 11 ] Available from: https://doi.org/10.1051/0004-6361/201526765
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
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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: 11 ago. 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 ago. 11 ] 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 ago. 11 ] Available from: https://doi.org/10.1051/0004-6361/201527558
Artigo de periodico
High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP1 (2016)
Barbuy, Beatriz Leonor Silveira; Cantelli, E; Vemado, A; Ernandes, H; Ortoloni, S; Saviane, I; Bica, E; Minniti, D; Dias, B; Momany, Y; Hill, V; Zoccali, M; Siqueira Mello, C
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, CENTRO GALÁCTICO
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ABNT
BARBUY, Beatriz Leonor Silveira et al. High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP1. Astronomy & Astrophysics, v. 591, p. A53/1-A53/14, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201628106. Acesso em: 11 ago. 2024.
APA
Barbuy, B. L. S., Cantelli, E., Vemado, A., Ernandes, H., Ortoloni, S., Saviane, I., et al. (2016). High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP1. Astronomy & Astrophysics, 591, A53/1-A53/14. doi:10.1051/0004-6361/201628106
NLM
Barbuy BLS, Cantelli E, Vemado A, Ernandes H, Ortoloni S, Saviane I, Bica E, Minniti D, Dias B, Momany Y, Hill V, Zoccali M, Siqueira Mello C. High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP1 [Internet]. Astronomy & Astrophysics. 2016 ;591 A53/1-A53/14.[citado 2024 ago. 11 ] Available from: https://doi.org/10.1051/0004-6361/201628106
Vancouver
Barbuy BLS, Cantelli E, Vemado A, Ernandes H, Ortoloni S, Saviane I, Bica E, Minniti D, Dias B, Momany Y, Hill V, Zoccali M, Siqueira Mello C. High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP1 [Internet]. Astronomy & Astrophysics. 2016 ;591 A53/1-A53/14.[citado 2024 ago. 11 ] Available from: https://doi.org/10.1051/0004-6361/201628106
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
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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: 11 ago. 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 ago. 11 ] 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 ago. 11 ] Available from: https://doi.org/10.1051/0004-6361/201527558
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)
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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: 11 ago. 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 ago. 11 ] 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 ago. 11 ] Available from: https://doi.org/10.1051/0004-6361/201423996
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: 11 ago. 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 ago. 11 ] 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 ago. 11 ] 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
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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: 11 ago. 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 ago. 11 ]
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 ago. 11 ]
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
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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: 11 ago. 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 ago. 11 ]
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 ago. 11 ]
Trabalho de evento-resumo
Metallicities and alpha-to-iron ratios in globular clusters stars on a homogeneous scale: search for multiple populations (2014)
Dias, B; Salviane, I; Barbuy, Beatriz Leonor Silveira; Held, E; Costa, G. S. da; Ortolani, S; Vasquez, S
Source: ASP Conference Series. Conference titles: Fifty Stars of Wide Field Studies in the Southern Hemisphere: Resolved Stellar Populations of the Galactic Bulge and Magellanic Clouds. Unidade: IAG
Subjects: AGLOMERADOS (GALÁXIA), COSMOQUÍMICA
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ABNT
DIAS, B et al. Metallicities and alpha-to-iron ratios in globular clusters stars on a homogeneous scale: search for multiple populations. 2014, Anais.. San Francisco: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, 2014. p. 134. . Acesso em: 11 ago. 2024.
APA
Dias, B., Salviane, I., Barbuy, B. L. S., Held, E., Costa, G. S. da, Ortolani, S., & Vasquez, S. (2014). Metallicities and alpha-to-iron ratios in globular clusters stars on a homogeneous scale: search for multiple populations. In ASP Conference Series (Vol. 491, p. 134). San Francisco: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo.
NLM
Dias B, Salviane I, Barbuy BLS, Held E, Costa GS da, Ortolani S, Vasquez S. Metallicities and alpha-to-iron ratios in globular clusters stars on a homogeneous scale: search for multiple populations. ASP Conference Series. 2014 ; 491 134.[citado 2024 ago. 11 ]
Vancouver
Dias B, Salviane I, Barbuy BLS, Held E, Costa GS da, Ortolani S, Vasquez S. Metallicities and alpha-to-iron ratios in globular clusters stars on a homogeneous scale: search for multiple populations. ASP Conference Series. 2014 ; 491 134.[citado 2024 ago. 11 ]
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
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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: 11 ago. 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 ago. 11 ]
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 ago. 11 ]
Artigo de periodico
VVV DR1: the first data release of the Milky Way bulge and southern plane from the near-infrared ESO public survey VISTA variables in the Vía Láctea (2012)
Saito, R. K; Barbuy, Beatriz Leonor Silveira; Dias, B; Sodré Júnior, Laerte
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), CENTRO GALÁCTICO, ESTRELAS, ABUNDÂNCIA ESTELAR, INFRAVERMELHO
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ABNT
SAITO, R. K et al. VVV DR1: the first data release of the Milky Way bulge and southern plane from the near-infrared ESO public survey VISTA variables in the Vía Láctea. Astronomy & Astrophysics, v. 537, p. A107/1-A107/21, 2012Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201118407. Acesso em: 11 ago. 2024.
APA
Saito, R. K., Barbuy, B. L. S., Dias, B., & Sodré Júnior, L. (2012). VVV DR1: the first data release of the Milky Way bulge and southern plane from the near-infrared ESO public survey VISTA variables in the Vía Láctea. Astronomy & Astrophysics, 537, A107/1-A107/21. doi:10.1051/0004-6361/201118407
NLM
Saito RK, Barbuy BLS, Dias B, Sodré Júnior L. VVV DR1: the first data release of the Milky Way bulge and southern plane from the near-infrared ESO public survey VISTA variables in the Vía Láctea [Internet]. Astronomy & Astrophysics. 2012 ; 537 A107/1-A107/21.[citado 2024 ago. 11 ] Available from: https://doi.org/10.1051/0004-6361/201118407
Vancouver
Saito RK, Barbuy BLS, Dias B, Sodré Júnior L. VVV DR1: the first data release of the Milky Way bulge and southern plane from the near-infrared ESO public survey VISTA variables in the Vía Láctea [Internet]. Astronomy & Astrophysics. 2012 ; 537 A107/1-A107/21.[citado 2024 ago. 11 ] Available from: https://doi.org/10.1051/0004-6361/201118407
Artigo de periodico
Milky Way demographics with the VVV survey: I. The 84-million star colour–magnitude diagram of the Galactic bulge (2012)
Saito, R. K; Minniti, D; Dias, B; Hempel, M; Rejkuba, M; Alonso-García, J; Barbuy, Beatriz Leonor Silveira; Catelan, M; Emerson, J. P; González, O. A; Lucas, P. W; Zoccali, M
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), CENTRO GALÁCTICO, ESTRUTURA DA GALÁXIA, ESTRELAS
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ABNT
SAITO, R. K et al. Milky Way demographics with the VVV survey: I. The 84-million star colour–magnitude diagram of the Galactic bulge. Astronomy & Astrophysics, v. 544, p. A147/1-A147/9, 2012Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201219448. Acesso em: 11 ago. 2024.
APA
Saito, R. K., Minniti, D., Dias, B., Hempel, M., Rejkuba, M., Alonso-García, J., et al. (2012). Milky Way demographics with the VVV survey: I. The 84-million star colour–magnitude diagram of the Galactic bulge. Astronomy & Astrophysics, 544, A147/1-A147/9. doi:10.1051/0004-6361/201219448
NLM
Saito RK, Minniti D, Dias B, Hempel M, Rejkuba M, Alonso-García J, Barbuy BLS, Catelan M, Emerson JP, González OA, Lucas PW, Zoccali M. Milky Way demographics with the VVV survey: I. The 84-million star colour–magnitude diagram of the Galactic bulge [Internet]. Astronomy & Astrophysics. 2012 ; 544 A147/1-A147/9.[citado 2024 ago. 11 ] Available from: https://doi.org/10.1051/0004-6361/201219448
Vancouver
Saito RK, Minniti D, Dias B, Hempel M, Rejkuba M, Alonso-García J, Barbuy BLS, Catelan M, Emerson JP, González OA, Lucas PW, Zoccali M. Milky Way demographics with the VVV survey: I. The 84-million star colour–magnitude diagram of the Galactic bulge [Internet]. Astronomy & Astrophysics. 2012 ; 544 A147/1-A147/9.[citado 2024 ago. 11 ] Available from: https://doi.org/10.1051/0004-6361/201219448
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
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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: 11 ago. 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 ago. 11 ] 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 ago. 11 ] Available from: https://doi.org/10.1017/s174392131000308x
Artigo de periodico
Metal-poor globular clusters of the Galactic bulge (2009)
Barbuy, Beatriz Leonor Silveira; Dias, B; Alves-Brito, A
Source: Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias). Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, GALÁXIA (VIA LÁCTEA)
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ABNT
BARBUY, Beatriz Leonor Silveira e DIAS, B e ALVES-BRITO, A. Metal-poor globular clusters of the Galactic bulge. Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias), v. 35, p. 150-151, 2009Tradução . . Disponível em: https://doi.org/10.1017/s1743921310000840. Acesso em: 11 ago. 2024.
APA
Barbuy, B. L. S., Dias, B., & Alves-Brito, A. (2009). Metal-poor globular clusters of the Galactic bulge. Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias), 35, 150-151. doi:10.1017/s1743921310000840
NLM
Barbuy BLS, Dias B, Alves-Brito A. Metal-poor globular clusters of the Galactic bulge [Internet]. Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias). 2009 ; 35 150-151.[citado 2024 ago. 11 ] Available from: https://doi.org/10.1017/s1743921310000840
Vancouver
Barbuy BLS, Dias B, Alves-Brito A. Metal-poor globular clusters of the Galactic bulge [Internet]. Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias). 2009 ; 35 150-151.[citado 2024 ago. 11 ] Available from: https://doi.org/10.1017/s1743921310000840

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