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Artigo de periodico
Another relic bulge globular cluster: ESO 456-SC38 (Djorgovski 2)⋆ (2019)
Ortolani, S; Barbuy, Beatriz Leonor Silveira
Source: Astronomy & Astrophysics. Unidade: IAG
Assunto: GALÁXIA (VIA LÁCTEA)
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ABNT
ORTOLANI, S e BARBUY, Beatriz Leonor Silveira. Another relic bulge globular cluster: ESO 456-SC38 (Djorgovski 2)⋆. Astronomy & Astrophysics, v. 627, p. A145, 2019Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201935726. Acesso em: 05 jun. 2024.
APA
Ortolani, S., & Barbuy, B. L. S. (2019). Another relic bulge globular cluster: ESO 456-SC38 (Djorgovski 2)⋆. Astronomy & Astrophysics, 627, A145. doi:10.1051/0004-6361/201935726
NLM
Ortolani S, Barbuy BLS. Another relic bulge globular cluster: ESO 456-SC38 (Djorgovski 2)⋆ [Internet]. Astronomy & Astrophysics. 2019 ; 627 A145.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201935726
Vancouver
Ortolani S, Barbuy BLS. Another relic bulge globular cluster: ESO 456-SC38 (Djorgovski 2)⋆ [Internet]. Astronomy & Astrophysics. 2019 ; 627 A145.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201935726
Artigo de periodico
J-PLUS: On the identiﬁcation of new cluster members in the double galaxy cluster A2589 & A2593 using PDFs (2019)
Molino, A; Oliveira, Claudia Lucia Mendes de; Cypriano, Eduardo Serra; Sodré Júnior, Laerte; Coelho, Patrícia; Monteiro-Oliveira, R; Sampedro, L; Schoenell, W; Hernández-Fernández, Jonathan D; Cortesi, Arianne; Cibirka, N; Novais, P; Pereira, E; Herández-Jimenez, J. A
Source: Astronomy & Astrophysics. Unidades: IAG, FFLCH
Subjects: FOTOMETRIA, INSTRUMENTAÇÃO (ASTRONOMIA), GALÁXIA (VIA LÁCTEA)
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ABNT
MOLINO, A et al. J-PLUS: On the identiﬁcation of new cluster members in the double galaxy cluster A2589 & A2593 using PDFs. Astronomy & Astrophysics, v. 622, p. A178, 2019Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201731348. Acesso em: 05 jun. 2024.
APA
Molino, A., Oliveira, C. L. M. de, Cypriano, E. S., Sodré Júnior, L., Coelho, P., Monteiro-Oliveira, R., et al. (2019). J-PLUS: On the identiﬁcation of new cluster members in the double galaxy cluster A2589 & A2593 using PDFs. Astronomy & Astrophysics, 622, A178. doi:10.1051/0004-6361/201731348
NLM
Molino A, Oliveira CLM de, Cypriano ES, Sodré Júnior L, Coelho P, Monteiro-Oliveira R, Sampedro L, Schoenell W, Hernández-Fernández JD, Cortesi A, Cibirka N, Novais P, Pereira E, Herández-Jimenez JA. J-PLUS: On the identiﬁcation of new cluster members in the double galaxy cluster A2589 & A2593 using PDFs [Internet]. Astronomy & Astrophysics. 2019 ; 622 A178.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201731348
Vancouver
Molino A, Oliveira CLM de, Cypriano ES, Sodré Júnior L, Coelho P, Monteiro-Oliveira R, Sampedro L, Schoenell W, Hernández-Fernández JD, Cortesi A, Cibirka N, Novais P, Pereira E, Herández-Jimenez JA. J-PLUS: On the identiﬁcation of new cluster members in the double galaxy cluster A2589 & A2593 using PDFs [Internet]. Astronomy & Astrophysics. 2019 ; 622 A178.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201731348
Artigo de periodico
The geometry of the magnetic field in the central molecular zone measured by PILOT (2019)
Mangilli, A; Dal Pino, Elisabete Maria de Gouveia ; Magalhães, Antonio Mário
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: CENTRO GALÁCTICO, GALÁXIA (VIA LÁCTEA), POLARIZAÇÃO (ASTRONOMIA)
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ABNT
MANGILLI, A e DAL PINO, Elisabete Maria de Gouveia e MAGALHÃES, Antonio Mário. The geometry of the magnetic field in the central molecular zone measured by PILOT. Astronomy & Astrophysics, v. 630, p. A74, 2019Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201935072. Acesso em: 05 jun. 2024.
APA
Mangilli, A., Dal Pino, E. M. de G., & Magalhães, A. M. (2019). The geometry of the magnetic field in the central molecular zone measured by PILOT. Astronomy & Astrophysics, 630, A74. doi:10.1051/0004-6361/201935072
NLM
Mangilli A, Dal Pino EM de G, Magalhães AM. The geometry of the magnetic field in the central molecular zone measured by PILOT [Internet]. Astronomy & Astrophysics. 2019 ; 630 A74.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201935072
Vancouver
Mangilli A, Dal Pino EM de G, Magalhães AM. The geometry of the magnetic field in the central molecular zone measured by PILOT [Internet]. Astronomy & Astrophysics. 2019 ; 630 A74.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201935072
Artigo de periodico
A MUSE study of the inner bulge globular cluster Terzan 9: a fossil record in the Galaxy⋆ (2019)
Ernandes, H; Barbuy, Beatriz Leonor Silveira
Source: Astronomy & Astrophysics. Unidade: IAG
Assunto: GALÁXIA (VIA LÁCTEA)
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ABNT
ERNANDES, H e BARBUY, Beatriz Leonor Silveira. A MUSE study of the inner bulge globular cluster Terzan 9: a fossil record in the Galaxy⋆. Astronomy & Astrophysics, v. 632, p. A103, 2019Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201936431. Acesso em: 05 jun. 2024.
APA
Ernandes, H., & Barbuy, B. L. S. (2019). A MUSE study of the inner bulge globular cluster Terzan 9: a fossil record in the Galaxy⋆. Astronomy & Astrophysics, 632, A103. doi:10.1051/0004-6361/201936431
NLM
Ernandes H, Barbuy BLS. A MUSE study of the inner bulge globular cluster Terzan 9: a fossil record in the Galaxy⋆ [Internet]. Astronomy & Astrophysics. 2019 ; 632 A103.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201936431
Vancouver
Ernandes H, Barbuy BLS. A MUSE study of the inner bulge globular cluster Terzan 9: a fossil record in the Galaxy⋆ [Internet]. Astronomy & Astrophysics. 2019 ; 632 A103.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201936431
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: 05 jun. 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 jun. 05 ] 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 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201833953
Artigo de periodico
Homogeneous metallicities and radial velocities for Galactic globular clusters: II. New CaT metallicities for 28 distant and reddened globular clusters (2018)
Vásquez, S; Saviane, I; Held, E. V; Da Costa, G. S; Dias, B; Gullieuszik, M; Barbuy, Beatriz Leonor Silveira; Ortolani, S; Zoccali, M
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR, GALÁXIA (VIA LÁCTEA)
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ABNT
VÁSQUEZ, S et al. Homogeneous metallicities and radial velocities for Galactic globular clusters: II. New CaT metallicities for 28 distant and reddened globular clusters. Astronomy & Astrophysics, v. 619, p. A13, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201833525. Acesso em: 05 jun. 2024.
APA
Vásquez, S., Saviane, I., Held, E. V., Da Costa, G. S., Dias, B., Gullieuszik, M., et al. (2018). Homogeneous metallicities and radial velocities for Galactic globular clusters: II. New CaT metallicities for 28 distant and reddened globular clusters. Astronomy & Astrophysics, 619, A13. doi:10.1051/0004-6361/201833525
NLM
Vásquez S, Saviane I, Held EV, Da Costa GS, Dias B, Gullieuszik M, Barbuy BLS, Ortolani S, Zoccali M. Homogeneous metallicities and radial velocities for Galactic globular clusters: II. New CaT metallicities for 28 distant and reddened globular clusters [Internet]. Astronomy & Astrophysics. 2018 ; 619 A13.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201833525
Vancouver
Vásquez S, Saviane I, Held EV, Da Costa GS, Dias B, Gullieuszik M, Barbuy BLS, Ortolani S, Zoccali M. Homogeneous metallicities and radial velocities for Galactic globular clusters: II. New CaT metallicities for 28 distant and reddened globular clusters [Internet]. Astronomy & Astrophysics. 2018 ; 619 A13.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201833525
Artigo de periodico
Modelling resonances and orbital chaos in disk galaxies - Application to a Milky Way spiral model (2017)
Michtchenko, Tatiana Alexandrovna; Vieira, R.S.S; Barros, D. A; Lépine, Jacques Raymond Daniel
Source: Astronomy and Astrophysysics. Unidade: IAG
Subjects: GALÁXIAS, GALÁXIA (VIA LÁCTEA)
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ABNT
MICHTCHENKO, Tatiana Alexandrovna et al. Modelling resonances and orbital chaos in disk galaxies - Application to a Milky Way spiral model. Astronomy and Astrophysysics, v. 597, p. A39, 2017Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201628895. Acesso em: 05 jun. 2024.
APA
Michtchenko, T. A., Vieira, R. S. S., Barros, D. A., & Lépine, J. R. D. (2017). Modelling resonances and orbital chaos in disk galaxies - Application to a Milky Way spiral model. Astronomy and Astrophysysics, 597, A39. doi:10.1051/0004-6361/201628895
NLM
Michtchenko TA, Vieira RSS, Barros DA, Lépine JRD. Modelling resonances and orbital chaos in disk galaxies - Application to a Milky Way spiral model [Internet]. Astronomy and Astrophysysics. 2017 ;597 A39.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201628895
Vancouver
Michtchenko TA, Vieira RSS, Barros DA, Lépine JRD. Modelling resonances and orbital chaos in disk galaxies - Application to a Milky Way spiral model [Internet]. Astronomy and Astrophysysics. 2017 ;597 A39.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201628895
Artigo de periodico
Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars (2016)
Spina, Lorenzo; Moreno, Jorge Luiz Meléndez; Ramírez, Iván
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ESTRELAS, PLANETAS, GALÁXIA (VIA LÁCTEA), FORMAÇÃO E EVOLUÇÃO DA GALÁXIA
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ABNT
SPINA, Lorenzo e MORENO, Jorge Luiz Meléndez e RAMÍREZ, Iván. Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars. Astronomy & Astrophysics, v. 585, p. A152/1-A152/15, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527429. Acesso em: 05 jun. 2024.
APA
Spina, L., Moreno, J. L. M., & Ramírez, I. (2016). Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars. Astronomy & Astrophysics, 585, A152/1-A152/15. doi:10.1051/0004-6361/201527429
NLM
Spina L, Moreno JLM, Ramírez I. Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars [Internet]. Astronomy & Astrophysics. 2016 ; 585 A152/1-A152/15.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201527429
Vancouver
Spina L, Moreno JLM, Ramírez I. Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars [Internet]. Astronomy & Astrophysics. 2016 ; 585 A152/1-A152/15.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201527429
Artigo de periodico
Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants (2016)
van der Swaelmen, M; Barbuy, Beatriz Leonor Silveira; Hill, V; Zoccali, M; Minniti, D; Ortolani, S; Gómez, A
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, GALÁXIA (VIA LÁCTEA)
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ABNT
VAN DER SWAELMEN, M et al. Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants. Astronomy & Astrophysics, v. 586, p. A1/1-A1/11, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201525709. Acesso em: 05 jun. 2024.
APA
van der Swaelmen, M., Barbuy, B. L. S., Hill, V., Zoccali, M., Minniti, D., Ortolani, S., & Gómez, A. (2016). Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants. Astronomy & Astrophysics, 586, A1/1-A1/11. doi:10.1051/0004-6361/201525709
NLM
van der Swaelmen M, Barbuy BLS, Hill V, Zoccali M, Minniti D, Ortolani S, Gómez A. Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants [Internet]. Astronomy & Astrophysics. 2016 ; 586 A1/1-A1/11.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201525709
Vancouver
van der Swaelmen M, Barbuy BLS, Hill V, Zoccali M, Minniti D, Ortolani S, Gómez A. Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants [Internet]. Astronomy & Astrophysics. 2016 ; 586 A1/1-A1/11.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201525709
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)
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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: 05 jun. 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 jun. 05 ] 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 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201527535
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: 05 jun. 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 jun. 05 ] 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 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201423996
Artigo de periodico
Zinc abundances in Galactic bulge field red giants: implications for damped Lyman-alpha systems (2015)
Barbuy, Beatriz Leonor Silveira; Friaça, Amâncio César Santos; Silveira, C. R. da; Hill, V; Zoccali, M; Minniti, D; Renzini, A; Ortolani, S; Gómez, A
Source: Astronomy & Astrophysics. Unidades: IAG, FO
Subjects: ABUNDÂNCIA ESTELAR, GALÁXIA (VIA LÁCTEA), GALÁXIAS (EVOLUÇÃO)
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ABNT
BARBUY, Beatriz Leonor Silveira et al. Zinc abundances in Galactic bulge field red giants: implications for damped Lyman-alpha systems. Astronomy & Astrophysics, v. 580, p. A40/1-A40/16, 2015Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201525694. Acesso em: 05 jun. 2024.
APA
Barbuy, B. L. S., Friaça, A. C. S., Silveira, C. R. da, Hill, V., Zoccali, M., Minniti, D., et al. (2015). Zinc abundances in Galactic bulge field red giants: implications for damped Lyman-alpha systems. Astronomy & Astrophysics, 580, A40/1-A40/16. doi:10.1051/0004-6361/201525694
NLM
Barbuy BLS, Friaça ACS, Silveira CR da, Hill V, Zoccali M, Minniti D, Renzini A, Ortolani S, Gómez A. Zinc abundances in Galactic bulge field red giants: implications for damped Lyman-alpha systems [Internet]. Astronomy & Astrophysics. 2015 ; 580 A40/1-A40/16.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201525694
Vancouver
Barbuy BLS, Friaça ACS, Silveira CR da, Hill V, Zoccali M, Minniti D, Renzini A, Ortolani S, Gómez A. Zinc abundances in Galactic bulge field red giants: implications for damped Lyman-alpha systems [Internet]. Astronomy & Astrophysics. 2015 ; 580 A40/1-A40/16.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201525694
Trabalho de evento-resumo
First stars inthe Galactic bulge? (2015)
Barbuy, Beatriz Leonor Silveira; Chiappini, Cristina
Source: Meeting Abstracts. Conference titles: IAU General Assembly. Unidade: IAG
Subjects: ESTRELAS, GALÁXIA (VIA LÁCTEA)
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ABNT
BARBUY, Beatriz Leonor Silveira e CHIAPPINI, Cristina. First stars inthe Galactic bulge? 2015, Anais.. Paris: International Astronomical Union, 2015. . Acesso em: 05 jun. 2024.
APA
Barbuy, B. L. S., & Chiappini, C. (2015). First stars inthe Galactic bulge? In Meeting Abstracts. Paris: International Astronomical Union.
NLM
Barbuy BLS, Chiappini C. First stars inthe Galactic bulge? Meeting Abstracts. 2015 ;[citado 2024 jun. 05 ]
Vancouver
Barbuy BLS, Chiappini C. First stars inthe Galactic bulge? Meeting Abstracts. 2015 ;[citado 2024 jun. 05 ]
Trabalho de evento-resumo
New eyes on the first stars: the old bulge component and the important role of PNe in this context (2015)
Chiappini, C; Cescutti, G; Barbuy, Beatriz Leonor Silveira; Meynet, G; Hirschi, R
Source: Meeting Abstracts. Conference titles: IAU General Assembly. Unidade: IAG
Subjects: ESTRELAS, ASTROQUÍMICA, GALÁXIA (VIA LÁCTEA)
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ABNT
CHIAPPINI, C et al. New eyes on the first stars: the old bulge component and the important role of PNe in this context. 2015, Anais.. Paris: International Astronomical Union, 2015. . Acesso em: 05 jun. 2024.
APA
Chiappini, C., Cescutti, G., Barbuy, B. L. S., Meynet, G., & Hirschi, R. (2015). New eyes on the first stars: the old bulge component and the important role of PNe in this context. In Meeting Abstracts. Paris: International Astronomical Union.
NLM
Chiappini C, Cescutti G, Barbuy BLS, Meynet G, Hirschi R. New eyes on the first stars: the old bulge component and the important role of PNe in this context. Meeting Abstracts. 2015 ;[citado 2024 jun. 05 ]
Vancouver
Chiappini C, Cescutti G, Barbuy BLS, Meynet G, Hirschi R. New eyes on the first stars: the old bulge component and the important role of PNe in this context. Meeting Abstracts. 2015 ;[citado 2024 jun. 05 ]
Artigo de periodico
High-resolution abundance analysis of very metal-poor r-I stars (2014)
Siqueira Mello, C.; Hill, V; Barbuy, Beatriz Leonor Silveira; Spite, M; Spite, F; Beers , T.C.; Caffau, E.; Bonifacio, P; Cayrel, R; François, P; Schatz, H; Wanajo, S
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), GALÁXIAS, ABUNDÂNCIA ESTELAR
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ABNT
SIQUEIRA MELLO, C. et al. High-resolution abundance analysis of very metal-poor r-I stars. Astronomy & Astrophysics, v. 565, p. A93/1-A93/23, 2014Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201423826. Acesso em: 05 jun. 2024.
APA
Siqueira Mello, C., Hill, V., Barbuy, B. L. S., Spite, M., Spite, F., Beers , T. C., et al. (2014). High-resolution abundance analysis of very metal-poor r-I stars. Astronomy & Astrophysics, 565, A93/1-A93/23. doi:10.1051/0004-6361/201423826
NLM
Siqueira Mello C, Hill V, Barbuy BLS, Spite M, Spite F, Beers TC, Caffau E, Bonifacio P, Cayrel R, François P, Schatz H, Wanajo S. High-resolution abundance analysis of very metal-poor r-I stars [Internet]. Astronomy & Astrophysics. 2014 ; 565 A93/1-A93/23.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201423826
Vancouver
Siqueira Mello C, Hill V, Barbuy BLS, Spite M, Spite F, Beers TC, Caffau E, Bonifacio P, Cayrel R, François P, Schatz H, Wanajo S. High-resolution abundance analysis of very metal-poor r-I stars [Internet]. Astronomy & Astrophysics. 2014 ; 565 A93/1-A93/23.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201423826
Artigo de periodico
High-resolution abundance analysis of red giants in the globular cluster NGC 6522 (2014)
Barbuy, Beatriz Leonor Silveira; Chiappini, C; Cantelli, E; Depagne, E; Pignatari, M; Hirschi, R; Cescutti, G; Ortolani, S; Hill, V; Zoccali, M; Minniti, D; Trevisan, M; Bica, E; Gómez, A
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, CENTRO GALÁCTICO, AGLOMERADOS (GALÁXIA), GALÁXIA (VIA LÁCTEA)
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
BARBUY, Beatriz Leonor Silveira et al. High-resolution abundance analysis of red giants in the globular cluster NGC 6522. Astronomy & Astrophysics, v. 570, p. A76/1-A76/21, 2014Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201424311. Acesso em: 05 jun. 2024.
APA
Barbuy, B. L. S., Chiappini, C., Cantelli, E., Depagne, E., Pignatari, M., Hirschi, R., et al. (2014). High-resolution abundance analysis of red giants in the globular cluster NGC 6522. Astronomy & Astrophysics, 570, A76/1-A76/21. doi:10.1051/0004-6361/201424311
NLM
Barbuy BLS, Chiappini C, Cantelli E, Depagne E, Pignatari M, Hirschi R, Cescutti G, Ortolani S, Hill V, Zoccali M, Minniti D, Trevisan M, Bica E, Gómez A. High-resolution abundance analysis of red giants in the globular cluster NGC 6522 [Internet]. Astronomy & Astrophysics. 2014 ; 570 A76/1-A76/21.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201424311
Vancouver
Barbuy BLS, Chiappini C, Cantelli E, Depagne E, Pignatari M, Hirschi R, Cescutti G, Ortolani S, Hill V, Zoccali M, Minniti D, Trevisan M, Bica E, Gómez A. High-resolution abundance analysis of red giants in the globular cluster NGC 6522 [Internet]. Astronomy & Astrophysics. 2014 ; 570 A76/1-A76/21.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201424311
Artigo de periodico
Manganese abundances in Galactic bulge red giants (2013)
Barbuy, Beatriz Leonor Silveira; Hill, V; Zocalli, M; Minniti, D; Renzini, A; Ortolani, S; Gómez, A; Trevisan, M; Dutra, N
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR, GALÁXIA (VIA LÁCTEA)
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
BARBUY, Beatriz Leonor Silveira et al. Manganese abundances in Galactic bulge red giants. Astronomy & Astrophysics, v. 559, p. A5/1-A5/14, 2013Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201322380. Acesso em: 05 jun. 2024.
APA
Barbuy, B. L. S., Hill, V., Zocalli, M., Minniti, D., Renzini, A., Ortolani, S., et al. (2013). Manganese abundances in Galactic bulge red giants. Astronomy & Astrophysics, 559, A5/1-A5/14. doi:10.1051/0004-6361/201322380
NLM
Barbuy BLS, Hill V, Zocalli M, Minniti D, Renzini A, Ortolani S, Gómez A, Trevisan M, Dutra N. Manganese abundances in Galactic bulge red giants [Internet]. Astronomy & Astrophysics. 2013 ; 559 A5/1-A5/14.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201322380
Vancouver
Barbuy BLS, Hill V, Zocalli M, Minniti D, Renzini A, Ortolani S, Gómez A, Trevisan M, Dutra N. Manganese abundances in Galactic bulge red giants [Internet]. Astronomy & Astrophysics. 2013 ; 559 A5/1-A5/14.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201322380
Trabalho de evento
The star formation rate in the inner Milky Way Galaxy (2013)
Cavichia, Oscar; Mollá, Mercedes; Costa, Roberto Dell'Aglio Dias da; Maciel, Walter Junqueira
Source: Molecular Gas, Dust, and Star Formation in Galaxies: Proceedings of IAU Symposium n. 292, 2012. Conference titles: IAU Symposium. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIAS (ASTRONOMIA), FORMAÇÃO E EVOLUÇÃO DA GALÁXIA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
CAVICHIA, Oscar et al. The star formation rate in the inner Milky Way Galaxy. 2013, Anais.. Paris: International Astronomical Union, 2013. Disponível em: https://doi.org/10.1017/S1743921313000586. Acesso em: 05 jun. 2024.
APA
Cavichia, O., Mollá, M., Costa, R. D. 'A. D. da, & Maciel, W. J. (2013). The star formation rate in the inner Milky Way Galaxy. In Molecular Gas, Dust, and Star Formation in Galaxies: Proceedings of IAU Symposium n. 292, 2012. Paris: International Astronomical Union. doi:10.1017/S1743921313000586
NLM
Cavichia O, Mollá M, Costa RD'AD da, Maciel WJ. The star formation rate in the inner Milky Way Galaxy [Internet]. Molecular Gas, Dust, and Star Formation in Galaxies: Proceedings of IAU Symposium n. 292, 2012. 2013 ;[citado 2024 jun. 05 ] Available from: https://doi.org/10.1017/S1743921313000586
Vancouver
Cavichia O, Mollá M, Costa RD'AD da, Maciel WJ. The star formation rate in the inner Milky Way Galaxy [Internet]. Molecular Gas, Dust, and Star Formation in Galaxies: Proceedings of IAU Symposium n. 292, 2012. 2013 ;[citado 2024 jun. 05 ] Available from: https://doi.org/10.1017/S1743921313000586
Trabalho de evento
Bimodal chemical evolution of the Galactic disk and the Barium abundance of Cepheids (2013)
Lépine, Jacques Raymond Daniel; Andrievky, Sergei; Barros, Douglas; Junqueira, Thiago C; Scarano Jr., Sergio
Source: Setting the scene for Gaia and LAMOST: Proceedings of IAU Symposium n. 298, 2013. Conference titles: IAU Symposium. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), GALÁXIAS ESPIRAIS, ESTRELAS, ABUNDÂNCIAS (ASTRONOMIA), FORMAÇÃO E EVOLUÇÃO DA GALÁXIA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
LÉPINE, Jacques Raymond Daniel et al. Bimodal chemical evolution of the Galactic disk and the Barium abundance of Cepheids. 2013, Anais.. Paris: International Astronomical Union, 2013. Disponível em: https://doi.org/10.1017/S174392131300625X. Acesso em: 05 jun. 2024.
APA
Lépine, J. R. D., Andrievky, S., Barros, D., Junqueira, T. C., & Scarano Jr., S. (2013). Bimodal chemical evolution of the Galactic disk and the Barium abundance of Cepheids. In Setting the scene for Gaia and LAMOST: Proceedings of IAU Symposium n. 298, 2013. Paris: International Astronomical Union. doi:10.1017/S174392131300625X
NLM
Lépine JRD, Andrievky S, Barros D, Junqueira TC, Scarano Jr. S. Bimodal chemical evolution of the Galactic disk and the Barium abundance of Cepheids [Internet]. Setting the scene for Gaia and LAMOST: Proceedings of IAU Symposium n. 298, 2013. 2013 ;[citado 2024 jun. 05 ] Available from: https://doi.org/10.1017/S174392131300625X
Vancouver
Lépine JRD, Andrievky S, Barros D, Junqueira TC, Scarano Jr. S. Bimodal chemical evolution of the Galactic disk and the Barium abundance of Cepheids [Internet]. Setting the scene for Gaia and LAMOST: Proceedings of IAU Symposium n. 298, 2013. 2013 ;[citado 2024 jun. 05 ] Available from: https://doi.org/10.1017/S174392131300625X
Artigo de periodico
A new model for gravitational potential perturbations in disks of spiral galaxies: an application to our Galaxy (2013)
Junqueira, T. C; Lépine, Jacques Raymond Daniel; Braga, C. A. S; Barros, D. A
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), DINÂMICA DA GALÁXIA, ESTRUTURA DA GALÁXIA, GALÁXIAS ESPIRAIS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
JUNQUEIRA, T. C et al. A new model for gravitational potential perturbations in disks of spiral galaxies: an application to our Galaxy. Astronomy & Astrophysics, v. 550, p. A91/1-A91/12, 2013Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201219769. Acesso em: 05 jun. 2024.
APA
Junqueira, T. C., Lépine, J. R. D., Braga, C. A. S., & Barros, D. A. (2013). A new model for gravitational potential perturbations in disks of spiral galaxies: an application to our Galaxy. Astronomy & Astrophysics, 550, A91/1-A91/12. doi:10.1051/0004-6361/201219769
NLM
Junqueira TC, Lépine JRD, Braga CAS, Barros DA. A new model for gravitational potential perturbations in disks of spiral galaxies: an application to our Galaxy [Internet]. Astronomy & Astrophysics. 2013 ; 550 A91/1-A91/12.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201219769
Vancouver
Junqueira TC, Lépine JRD, Braga CAS, Barros DA. A new model for gravitational potential perturbations in disks of spiral galaxies: an application to our Galaxy [Internet]. Astronomy & Astrophysics. 2013 ; 550 A91/1-A91/12.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201219769

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