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OLIVEIRA, Yuri. Análise do perfil qiomiodinâmico da sobredensidade Triangulum-Andromeda. 2023. Dissertação (Mestrado) – Universidade de São Paulo, São Paulo, 2023. . Acesso em: 25 abr. 2026.
APA
Oliveira, Y. (2023). Análise do perfil qiomiodinâmico da sobredensidade Triangulum-Andromeda (Dissertação (Mestrado). Universidade de São Paulo, São Paulo.
NLM
Oliveira Y. Análise do perfil qiomiodinâmico da sobredensidade Triangulum-Andromeda. 2023 ;[citado 2026 abr. 25 ]
Vancouver
Oliveira Y. Análise do perfil qiomiodinâmico da sobredensidade Triangulum-Andromeda. 2023 ;[citado 2026 abr. 25 ]
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NOVAIS, P.M e SODRÉ JÚNIOR, Laerte. The morphology of Hα emission in CALIFA galaxies. Monthly Notices of the Royal Astronomical Society, v. 482, n. 2, p. 2717-2730, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty2855. Acesso em: 25 abr. 2026.
APA
Novais, P. M., & Sodré Júnior, L. (2019). The morphology of Hα emission in CALIFA galaxies. Monthly Notices of the Royal Astronomical Society, 482( 2), 2717-2730. doi:10.1093/mnras/sty2855
NLM
Novais PM, Sodré Júnior L. The morphology of Hα emission in CALIFA galaxies [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 482( 2): 2717-2730.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1093/mnras/sty2855
Vancouver
Novais PM, Sodré Júnior L. The morphology of Hα emission in CALIFA galaxies [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 482( 2): 2717-2730.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1093/mnras/sty2855
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LEAMAN, Ryan e COELHO, Paula Rodrigues Teixeira. Survival of molecular gas in a stellar feedback-driven outflow witnessed with the MUSE TIMER project and ALMA. Monthly Notices of the Royal Astronomical Society, v. 488, n. 3, p. 3904-3928, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz1844. Acesso em: 25 abr. 2026.
APA
Leaman, R., & Coelho, P. R. T. (2019). Survival of molecular gas in a stellar feedback-driven outflow witnessed with the MUSE TIMER project and ALMA. Monthly Notices of the Royal Astronomical Society, 488( 3), 3904-3928. doi:10.1093/mnras/stz1844
NLM
Leaman R, Coelho PRT. Survival of molecular gas in a stellar feedback-driven outflow witnessed with the MUSE TIMER project and ALMA [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 488( 3): 3904-3928.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1093/mnras/stz1844
Vancouver
Leaman R, Coelho PRT. Survival of molecular gas in a stellar feedback-driven outflow witnessed with the MUSE TIMER project and ALMA [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 488( 3): 3904-3928.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1093/mnras/stz1844
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MICHTCHENKO, Tatiana Alexandrovna et al. Moving Groups as the Origin of the Vertical Phase-space Spiral in the Galactic Neighborhood. The Astrophysical Journal, v. 876, n. 1, p. 36/1-36/7, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab11cd. Acesso em: 25 abr. 2026.
APA
Michtchenko, T. A., Barros, D. A., Perez-Villegas, A., & Lépine, J. R. D. (2019). Moving Groups as the Origin of the Vertical Phase-space Spiral in the Galactic Neighborhood. The Astrophysical Journal, 876( 1), 36/1-36/7. doi:10.3847/1538-4357/ab11cd
NLM
Michtchenko TA, Barros DA, Perez-Villegas A, Lépine JRD. Moving Groups as the Origin of the Vertical Phase-space Spiral in the Galactic Neighborhood [Internet]. The Astrophysical Journal. 2019 ; 876( 1): 36/1-36/7.[citado 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab11cd
Vancouver
Michtchenko TA, Barros DA, Perez-Villegas A, Lépine JRD. Moving Groups as the Origin of the Vertical Phase-space Spiral in the Galactic Neighborhood [Internet]. The Astrophysical Journal. 2019 ; 876( 1): 36/1-36/7.[citado 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab11cd
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LORENZO-CÁCERES, Adriana de e GADOTTI, Dimitri Alexei e COELHO, Paula Rodrigues Teixeira. Clocking the assembly of double-barred galaxies with the MUSE TIMER project. Monthly Notices of the Royal Astronomical Society, v. 484, n. 4, p. 5296-5314, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz221. Acesso em: 25 abr. 2026.
APA
Lorenzo-Cáceres, A. de, Gadotti, D. A., & Coelho, P. R. T. (2019). Clocking the assembly of double-barred galaxies with the MUSE TIMER project. Monthly Notices of the Royal Astronomical Society, 484( 4), 5296-5314. doi:10.1093/mnras/stz221
NLM
Lorenzo-Cáceres A de, Gadotti DA, Coelho PRT. Clocking the assembly of double-barred galaxies with the MUSE TIMER project [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 484( 4): 5296-5314.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1093/mnras/stz221
Vancouver
Lorenzo-Cáceres A de, Gadotti DA, Coelho PRT. Clocking the assembly of double-barred galaxies with the MUSE TIMER project [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 484( 4): 5296-5314.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1093/mnras/stz221
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DIAS, Wilton da Silva et al. The spiral pattern rotation speed of the Galaxy and the corotation radius with Gaia DR2. Monthly Notices of the Royal Astronomical Society, v. 486, n. 4, p. 5726-5736, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz1196. Acesso em: 25 abr. 2026.
APA
Dias, W. da S., Monteiro, H., Lépine, J. R. D., & Barros, D. A. (2019). The spiral pattern rotation speed of the Galaxy and the corotation radius with Gaia DR2. Monthly Notices of the Royal Astronomical Society, 486( 4), 5726-5736. doi:10.1093/mnras/stz1196
NLM
Dias W da S, Monteiro H, Lépine JRD, Barros DA. The spiral pattern rotation speed of the Galaxy and the corotation radius with Gaia DR2 [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 486( 4): 5726-5736.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1093/mnras/stz1196
Vancouver
Dias W da S, Monteiro H, Lépine JRD, Barros DA. The spiral pattern rotation speed of the Galaxy and the corotation radius with Gaia DR2 [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 486( 4): 5726-5736.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1093/mnras/stz1196
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GADOTTI, Dimitri A e COELHO, Paula Rodrigues Teixeira. Time Inference with MUSE in Extragalactic Rings (TIMER): properties of the survey and high-level data products. Monthly Notices of the Royal Astronomical Society, v. 482, n. 1, p. 506-529, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty2666. Acesso em: 25 abr. 2026.
APA
Gadotti, D. A., & Coelho, P. R. T. (2019). Time Inference with MUSE in Extragalactic Rings (TIMER): properties of the survey and high-level data products. Monthly Notices of the Royal Astronomical Society, 482( 1), 506-529. doi:10.1093/mnras/sty2666
NLM
Gadotti DA, Coelho PRT. Time Inference with MUSE in Extragalactic Rings (TIMER): properties of the survey and high-level data products [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 482( 1): 506-529.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1093/mnras/sty2666
Vancouver
Gadotti DA, Coelho PRT. Time Inference with MUSE in Extragalactic Rings (TIMER): properties of the survey and high-level data products [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 482( 1): 506-529.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1093/mnras/sty2666
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MICHTCHENKO, Tatiana Alexandrovna et al. On the Stellar Velocity Distribution in the Solar Neighborhood in Light of Gaia DR2. Astrophysical Journal Letters, v. 863, n. 2, p. L37-1-L37-6, 2018Tradução . . Disponível em: https://doi.org/10.3847/2041-8213/aad804. Acesso em: 25 abr. 2026.
APA
Michtchenko, T. A., Lépine, J. R. D., Perez-Villegas, A., Vieira, R. S. S., & Barros, D. A. (2018). On the Stellar Velocity Distribution in the Solar Neighborhood in Light of Gaia DR2. Astrophysical Journal Letters, 863( 2), L37-1-L37-6. doi:10.3847/2041-8213/aad804
NLM
Michtchenko TA, Lépine JRD, Perez-Villegas A, Vieira RSS, Barros DA. On the Stellar Velocity Distribution in the Solar Neighborhood in Light of Gaia DR2 [Internet]. Astrophysical Journal Letters. 2018 ; 863( 2): L37-1-L37-6.[citado 2026 abr. 25 ] Available from: https://doi.org/10.3847/2041-8213/aad804
Vancouver
Michtchenko TA, Lépine JRD, Perez-Villegas A, Vieira RSS, Barros DA. On the Stellar Velocity Distribution in the Solar Neighborhood in Light of Gaia DR2 [Internet]. Astrophysical Journal Letters. 2018 ; 863( 2): L37-1-L37-6.[citado 2026 abr. 25 ] Available from: https://doi.org/10.3847/2041-8213/aad804
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BARBOSA, C. E et al. Sloshing in its cD halo: MUSE kinematics of the central galaxy NGC 3311 in the Hydra I cluster. Astronomy & Astrophysics, v. 609, p. A78, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201731834. Acesso em: 25 abr. 2026.
APA
Barbosa, C. E., Arnaboldi, M., Coccato, L., Gerhard, O., Oliveira, C. L. M. de, Hilker, M., & Richtler, T. (2018). Sloshing in its cD halo: MUSE kinematics of the central galaxy NGC 3311 in the Hydra I cluster. Astronomy & Astrophysics, 609, A78. doi:10.1051/0004-6361/201731834
NLM
Barbosa CE, Arnaboldi M, Coccato L, Gerhard O, Oliveira CLM de, Hilker M, Richtler T. Sloshing in its cD halo: MUSE kinematics of the central galaxy NGC 3311 in the Hydra I cluster [Internet]. Astronomy & Astrophysics. 2018 ; 609 A78.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1051/0004-6361/201731834
Vancouver
Barbosa CE, Arnaboldi M, Coccato L, Gerhard O, Oliveira CLM de, Hilker M, Richtler T. Sloshing in its cD halo: MUSE kinematics of the central galaxy NGC 3311 in the Hydra I cluster [Internet]. Astronomy & Astrophysics. 2018 ; 609 A78.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1051/0004-6361/201731834
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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: 25 abr. 2026.
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 2026 abr. 25 ] 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 2026 abr. 25 ] Available from: https://doi.org/10.1051/0004-6361/201527535
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BEERS, Timothy C et al. Population studies: XIII. A new analysis of the Bidelman-MacConnell "weak-metal" stars - confirmation of metal-poor stars in the thick disk of the Galaxy. The Astrophysical Journal, v. 794, p. 58/1-58/19, 2014Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/794/1/58. Acesso em: 25 abr. 2026.
APA
Beers, T. C., Norris, J. E., Placco, V. M., Lee, Y. S., Rossi, S. C. F., Carollo, D., & Masseron, T. (2014). Population studies: XIII. A new analysis of the Bidelman-MacConnell "weak-metal" stars - confirmation of metal-poor stars in the thick disk of the Galaxy. The Astrophysical Journal, 794, 58/1-58/19. doi:10.1088/0004-637X/794/1/58
NLM
Beers TC, Norris JE, Placco VM, Lee YS, Rossi SCF, Carollo D, Masseron T. Population studies: XIII. A new analysis of the Bidelman-MacConnell "weak-metal" stars - confirmation of metal-poor stars in the thick disk of the Galaxy [Internet]. The Astrophysical Journal. 2014 ; 794 58/1-58/19.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1088/0004-637X/794/1/58
Vancouver
Beers TC, Norris JE, Placco VM, Lee YS, Rossi SCF, Carollo D, Masseron T. Population studies: XIII. A new analysis of the Bidelman-MacConnell "weak-metal" stars - confirmation of metal-poor stars in the thick disk of the Galaxy [Internet]. The Astrophysical Journal. 2014 ; 794 58/1-58/19.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1088/0004-637X/794/1/58
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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: 25 abr. 2026.
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 2026 abr. 25 ] 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 2026 abr. 25 ] Available from: https://doi.org/10.1051/0004-6361/201219769
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BARROS, D. A e LÉPINE, Jacques Raymond Daniel e JUNQUEIRA, T. C. A galactic ring of minimum stellar density near the solar orbit radius. Monthly Notices of the Royal Astronomical Society, p. 2299-2321, 2013Tradução . . Disponível em: https://doi.org/10.1093/mnras/stt1454. Acesso em: 25 abr. 2026.
APA
Barros, D. A., Lépine, J. R. D., & Junqueira, T. C. (2013). A galactic ring of minimum stellar density near the solar orbit radius. Monthly Notices of the Royal Astronomical Society, 2299-2321. doi:10.1093/mnras/stt1454
NLM
Barros DA, Lépine JRD, Junqueira TC. A galactic ring of minimum stellar density near the solar orbit radius [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 2299-2321.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1093/mnras/stt1454
Vancouver
Barros DA, Lépine JRD, Junqueira TC. A galactic ring of minimum stellar density near the solar orbit radius [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 2299-2321.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1093/mnras/stt1454
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POLIDO, P e JABLONSKI, F e LÉPINE, Jacques Raymond Daniel. A galaxy model from Two Micron All Sky Survey star counts in the whole sky, including the plane. The Astrophysical Journal, v. 778, n. 32, p. 1-18, 2013Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/778/1/32. Acesso em: 25 abr. 2026.
APA
Polido, P., Jablonski, F., & Lépine, J. R. D. (2013). A galaxy model from Two Micron All Sky Survey star counts in the whole sky, including the plane. The Astrophysical Journal, 778( 32), 1-18. doi:10.1088/0004-637X/778/1/32
NLM
Polido P, Jablonski F, Lépine JRD. A galaxy model from Two Micron All Sky Survey star counts in the whole sky, including the plane [Internet]. The Astrophysical Journal. 2013 ; 778( 32): 1-18.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1088/0004-637X/778/1/32
Vancouver
Polido P, Jablonski F, Lépine JRD. A galaxy model from Two Micron All Sky Survey star counts in the whole sky, including the plane [Internet]. The Astrophysical Journal. 2013 ; 778( 32): 1-18.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1088/0004-637X/778/1/32
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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POLIDO, P e JABLONSKI, F e LÉPINE, Jacques Raymond Daniel. A galaxy model from Two Micron All Sky Survey stars counts in the whole sky, including the plane. The Astrophysical Journal, v. 778, p. 32/1-32/18, 2013Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/778/1/32. Acesso em: 25 abr. 2026.
APA
Polido, P., Jablonski, F., & Lépine, J. R. D. (2013). A galaxy model from Two Micron All Sky Survey stars counts in the whole sky, including the plane. The Astrophysical Journal, 778, 32/1-32/18. doi:10.1088/0004-637X/778/1/32
NLM
Polido P, Jablonski F, Lépine JRD. A galaxy model from Two Micron All Sky Survey stars counts in the whole sky, including the plane [Internet]. The Astrophysical Journal. 2013 ; 778 32/1-32/18.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1088/0004-637X/778/1/32
Vancouver
Polido P, Jablonski F, Lépine JRD. A galaxy model from Two Micron All Sky Survey stars counts in the whole sky, including the plane [Internet]. The Astrophysical Journal. 2013 ; 778 32/1-32/18.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1088/0004-637X/778/1/32
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COSTA, Roberto Dell'Aglio Dias da e CAVICHIA, Oscar e MACIEL, Walter Junqueira. Planetary nebulae and determination of the bulge–disk boundary. 2013, Anais.. Paris: International Astronomical Union, 2013. Disponível em: https://doi.org/10.1017/S1743921312021746. Acesso em: 25 abr. 2026.
APA
Costa, R. D. 'A. D. da, Cavichia, O., & Maciel, W. J. (2013). Planetary nebulae and determination of the bulge–disk boundary. In Advancing the Physics of Cosmic Distances: Proceedings of IAU Symposium n. 289, 2012. Paris: International Astronomical Union. doi:10.1017/S1743921312021746
NLM
Costa RD'AD da, Cavichia O, Maciel WJ. Planetary nebulae and determination of the bulge–disk boundary [Internet]. Advancing the Physics of Cosmic Distances: Proceedings of IAU Symposium n. 289, 2012. 2013 ;[citado 2026 abr. 25 ] Available from: https://doi.org/10.1017/S1743921312021746
Vancouver
Costa RD'AD da, Cavichia O, Maciel WJ. Planetary nebulae and determination of the bulge–disk boundary [Internet]. Advancing the Physics of Cosmic Distances: Proceedings of IAU Symposium n. 289, 2012. 2013 ;[citado 2026 abr. 25 ] Available from: https://doi.org/10.1017/S1743921312021746
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AMÔRES, E. B et al. Galaxies behind the galactic plane: first results and perspectives from the VVV survey. The Astronomical Journal, v. 144, p. 127/1-127/11, 2012Tradução . . Disponível em: https://doi.org/10.1088/0004-6256/144/5/127. Acesso em: 25 abr. 2026.
APA
Amôres, E. B., Sodré Júnior, L., Minniti, D., Alonso, M. V., Padilla, N., Gurovich, S., et al. (2012). Galaxies behind the galactic plane: first results and perspectives from the VVV survey. The Astronomical Journal, 144, 127/1-127/11. doi:10.1088/0004-6256/144/5/127
NLM
Amôres EB, Sodré Júnior L, Minniti D, Alonso MV, Padilla N, Gurovich S, Arsenijevic V, Tollerud EJ, Rodríguez-Ardila A, Díaz Tello J, Lucas W. Galaxies behind the galactic plane: first results and perspectives from the VVV survey [Internet]. The Astronomical Journal. 2012 ; 144 127/1-127/11.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1088/0004-6256/144/5/127
Vancouver
Amôres EB, Sodré Júnior L, Minniti D, Alonso MV, Padilla N, Gurovich S, Arsenijevic V, Tollerud EJ, Rodríguez-Ardila A, Díaz Tello J, Lucas W. Galaxies behind the galactic plane: first results and perspectives from the VVV survey [Internet]. The Astronomical Journal. 2012 ; 144 127/1-127/11.[citado 2026 abr. 25 ] Available from: https://doi.org/10.1088/0004-6256/144/5/127
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ACHAROVA, I. A e LÉPINE, Jacques Raymond Daniel e MISHUROV, Yu. N. Galactic corotation as a principal "driver'' for the formation of bimodal abundance radial distribution in the disk of our Galaxy. Astronomical & Astrophysical Transactions, v. 27, n. 2, p. 359-364, 2012Tradução . . Acesso em: 25 abr. 2026.
APA
Acharova, I. A., Lépine, J. R. D., & Mishurov, Y. N. (2012). Galactic corotation as a principal "driver'' for the formation of bimodal abundance radial distribution in the disk of our Galaxy. Astronomical & Astrophysical Transactions, 27( 2), 359-364.
NLM
Acharova IA, Lépine JRD, Mishurov YN. Galactic corotation as a principal "driver'' for the formation of bimodal abundance radial distribution in the disk of our Galaxy. Astronomical & Astrophysical Transactions. 2012 ; 27( 2): 359-364.[citado 2026 abr. 25 ]
Vancouver
Acharova IA, Lépine JRD, Mishurov YN. Galactic corotation as a principal "driver'' for the formation of bimodal abundance radial distribution in the disk of our Galaxy. Astronomical & Astrophysical Transactions. 2012 ; 27( 2): 359-364.[citado 2026 abr. 25 ]
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GALLI, Phillip Andreas Bernner. "Determinação de distâncias cinémáticas de estrelas pré-sequência principal em regiões de formação estelar". 2012. Tese (Doutorado) – Universidade de São Paulo, São Paulo, 2012. . Acesso em: 25 abr. 2026.
APA
Galli, P. A. B. (2012). "Determinação de distâncias cinémáticas de estrelas pré-sequência principal em regiões de formação estelar" (Tese (Doutorado). Universidade de São Paulo, São Paulo.
NLM
Galli PAB. "Determinação de distâncias cinémáticas de estrelas pré-sequência principal em regiões de formação estelar". 2012 ;[citado 2026 abr. 25 ]
Vancouver
Galli PAB. "Determinação de distâncias cinémáticas de estrelas pré-sequência principal em regiões de formação estelar". 2012 ;[citado 2026 abr. 25 ]
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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: 25 abr. 2026.
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 2026 abr. 25 ] 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 2026 abr. 25 ] Available from: https://doi.org/10.1051/0004-6361/201219448
