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Artigo de periodico
The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters (2020)
Oliveira, R. A. P. ; Souza, S. O ; keber, L. O ; Barbuy, Beatriz Leonor Silveira
Source: The Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), ATMOSFERAS ESTELARES, POPULAÇÕES ESTELARES
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ABNT
OLIVEIRA, R. A. P. et al. The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters. The Astrophysical Journal, v. No, n. 1, p. 28/1-28/23, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab6f76. Acesso em: 05 nov. 2024.
APA
Oliveira, R. A. P., Souza, S. O., keber, L. O., & Barbuy, B. L. S. (2020). The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters. The Astrophysical Journal, No( 1), 28/1-28/23. doi:10.3847/1538-4357/ab6f76
NLM
Oliveira RAP, Souza SO, keber LO, Barbuy BLS. The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters [Internet]. The Astrophysical Journal. 2020 ; No( 1): 28/1-28/23.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab6f76
Vancouver
Oliveira RAP, Souza SO, keber LO, Barbuy BLS. The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters [Internet]. The Astrophysical Journal. 2020 ; No( 1): 28/1-28/23.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab6f76
Artigo de periodico
Spatially resolved analysis of neutral winds, stars, and ionized gas kinematics with megara/gtc: new insights on the nearby galaxy ugc 10205 (2020)
Catalán-Torrecill, C ; Castilho-Morales, Á ; Coelho, Paula Rodrigues Teixeira
Source: The Astrophysical Journal. Unidade: IAG
Subjects: MEIO INTERESTELAR, ESPECTROSCOPIA
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CATALÁN-TORRECILL, C e CASTILHO-MORALES, Á e COELHO, Paula Rodrigues Teixeira. Spatially resolved analysis of neutral winds, stars, and ionized gas kinematics with megara/gtc: new insights on the nearby galaxy ugc 10205. The Astrophysical Journal, v. 890, p. 5, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab63ca. Acesso em: 05 nov. 2024.
APA
Catalán-Torrecill, C., Castilho-Morales, Á., & Coelho, P. R. T. (2020). Spatially resolved analysis of neutral winds, stars, and ionized gas kinematics with megara/gtc: new insights on the nearby galaxy ugc 10205. The Astrophysical Journal, 890, 5. doi:10.3847/1538-4357/ab63ca
NLM
Catalán-Torrecill C, Castilho-Morales Á, Coelho PRT. Spatially resolved analysis of neutral winds, stars, and ionized gas kinematics with megara/gtc: new insights on the nearby galaxy ugc 10205 [Internet]. The Astrophysical Journal. 2020 ; 890 5.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab63ca
Vancouver
Catalán-Torrecill C, Castilho-Morales Á, Coelho PRT. Spatially resolved analysis of neutral winds, stars, and ionized gas kinematics with megara/gtc: new insights on the nearby galaxy ugc 10205 [Internet]. The Astrophysical Journal. 2020 ; 890 5.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab63ca
Artigo de periodico
Self-consistent analysis of stellar clusters: an application to HST data of the halo globular cluster (2020)
Souza, S. O ; Kerber, Leandro de Oliveira ; Barbuy, Beatriz Leonor Silveira ; Pérez-Villegas, A ; Oliveira, R. A. P. ; Nardiello, D
Source: The Astrophysical Journal. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, POPULAÇÕES ESTELARES
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ABNT
SOUZA, S. O et al. Self-consistent analysis of stellar clusters: an application to HST data of the halo globular cluster. The Astrophysical Journal, v. 890, p. 13 2020, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab6a0f. Acesso em: 05 nov. 2024.
APA
Souza, S. O., Kerber, L. de O., Barbuy, B. L. S., Pérez-Villegas, A., Oliveira, R. A. P., & Nardiello, D. (2020). Self-consistent analysis of stellar clusters: an application to HST data of the halo globular cluster. The Astrophysical Journal, 890, 13 2020. doi:10.3847/1538-4357/ab6a0f
NLM
Souza SO, Kerber L de O, Barbuy BLS, Pérez-Villegas A, Oliveira RAP, Nardiello D. Self-consistent analysis of stellar clusters: an application to HST data of the halo globular cluster [Internet]. The Astrophysical Journal. 2020 ; 890 13 2020.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab6a0f
Vancouver
Souza SO, Kerber L de O, Barbuy BLS, Pérez-Villegas A, Oliveira RAP, Nardiello D. Self-consistent analysis of stellar clusters: an application to HST data of the halo globular cluster [Internet]. The Astrophysical Journal. 2020 ; 890 13 2020.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab6a0f
Artigo de periodico
Moving Groups as the Origin of the Vertical Phase-space Spiral in the Galactic Neighborhood (2019)
Michtchenko, Tatiana Alexandrovna; Barros, Douglas A; Perez-Villegas, Angeles; Lépine, Jacques Raymond Daniel
Source: The Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIAS ESPIRAIS, ESTRUTURA DA GALÁXIA
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ABNT
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: 05 nov. 2024.
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 2024 nov. 05 ] 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 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab11cd
Artigo de periodico
Very-high-energy Emission from Magnetic Reconnection in the Radiative-inefficient Accretion Flow of SgrA{*} (2019)
Rodríguez-Ramírez, Juan Carlos ; Dal Pino, Elisabete Maria de Gouveia ; Batista, Rafael Alves
Source: The Astrophysical Journal. Unidade: IAG
Subjects: DISCOS DE ACRESÇÃO, MAGNETOHIDRODINÂMICA, CENTRO GALÁCTICO
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ABNT
RODRÍGUEZ-RAMÍREZ, Juan Carlos e DAL PINO, Elisabete Maria de Gouveia e BATISTA, Rafael Alves. Very-high-energy Emission from Magnetic Reconnection in the Radiative-inefficient Accretion Flow of SgrA{*}. The Astrophysical Journal, v. 879, n. 1, p. 6/1-6/10, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab212e. Acesso em: 05 nov. 2024.
APA
Rodríguez-Ramírez, J. C., Dal Pino, E. M. de G., & Batista, R. A. (2019). Very-high-energy Emission from Magnetic Reconnection in the Radiative-inefficient Accretion Flow of SgrA{*}. The Astrophysical Journal, 879( 1), 6/1-6/10. doi:10.3847/1538-4357/ab212e
NLM
Rodríguez-Ramírez JC, Dal Pino EM de G, Batista RA. Very-high-energy Emission from Magnetic Reconnection in the Radiative-inefficient Accretion Flow of SgrA{*} [Internet]. The Astrophysical Journal. 2019 ; 879( 1): 6/1-6/10.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab212e
Vancouver
Rodríguez-Ramírez JC, Dal Pino EM de G, Batista RA. Very-high-energy Emission from Magnetic Reconnection in the Radiative-inefficient Accretion Flow of SgrA{*} [Internet]. The Astrophysical Journal. 2019 ; 879( 1): 6/1-6/10.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab212e
Artigo de periodico
First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release (2019)
Brout, D ; Lima, Marcos Vinicius Borges Teixeira
Source: The Astrophysical Journal. Unidade: IF
Subjects: COSMOLOGIA, MATÉRIA ESCURA, SUPERNOVAS
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ABNT
BROUT, D e LIMA, Marcos Vinicius Borges Teixeira. First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release. The Astrophysical Journal, v. 874, n. 1, p. 106/1-106/12, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab06c1. Acesso em: 05 nov. 2024.
APA
Brout, D., & Lima, M. V. B. T. (2019). First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release. The Astrophysical Journal, 874( 1), 106/1-106/12. doi:10.3847/1538-4357/ab06c1
NLM
Brout D, Lima MVBT. First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release [Internet]. The Astrophysical Journal. 2019 ; 874( 1): 106/1-106/12.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab06c1
Vancouver
Brout D, Lima MVBT. First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release [Internet]. The Astrophysical Journal. 2019 ; 874( 1): 106/1-106/12.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab06c1
Artigo de periodico
Nonlinear Rossby Wave-Wave and Wave-Mean Flow Theory for Long-term Solar Cycle Modulations (2019)
Raphaldini, Breno; Teruya, Andre Seiji; Raupp, Carlos Frederico Mendonça ; Bustamante, Miguel D
Source: The Astrophysical Journal. Unidade: IAG
Subjects: MAGNETOHIDRODINÂMICA, ONDAS DE ROSSBY, ATIVIDADE SOLAR
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ABNT
RAPHALDINI, Breno et al. Nonlinear Rossby Wave-Wave and Wave-Mean Flow Theory for Long-term Solar Cycle Modulations. The Astrophysical Journal, v. 887, n. 1, p. 17, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab5067. Acesso em: 05 nov. 2024.
APA
Raphaldini, B., Teruya, A. S., Raupp, C. F. M., & Bustamante, M. D. (2019). Nonlinear Rossby Wave-Wave and Wave-Mean Flow Theory for Long-term Solar Cycle Modulations. The Astrophysical Journal, 887( 1), 17. doi:10.3847/1538-4357/ab5067
NLM
Raphaldini B, Teruya AS, Raupp CFM, Bustamante MD. Nonlinear Rossby Wave-Wave and Wave-Mean Flow Theory for Long-term Solar Cycle Modulations [Internet]. The Astrophysical Journal. 2019 ; 887( 1): 17.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab5067
Vancouver
Raphaldini B, Teruya AS, Raupp CFM, Bustamante MD. Nonlinear Rossby Wave-Wave and Wave-Mean Flow Theory for Long-term Solar Cycle Modulations [Internet]. The Astrophysical Journal. 2019 ; 887( 1): 17.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab5067
Artigo de periodico
The discreteness-driven relaxation of collisionless gravitating systems: entropy evolution in external potentials, n-dependence and the role of chaos (2019)
Silva, Leandro Beraldo e; De Siqueira Pedra, Walter ; Valluri, Monica; Sodré Júnior, Laerte; Bru, Jean-Bernard
Source: The Astrophysical Journal. Unidades: IAG, IF
Subjects: GALÁXIAS, MECÂNICA QUÂNTICA, MATEMÁTICA APLICADA, COSMOLOGIA
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ABNT
SILVA, Leandro Beraldo e et al. The discreteness-driven relaxation of collisionless gravitating systems: entropy evolution in external potentials, n-dependence and the role of chaos. The Astrophysical Journal, v. 870, n. 2, p. 128, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aaf397. Acesso em: 05 nov. 2024.
APA
Silva, L. B. e, De Siqueira Pedra, W., Valluri, M., Sodré Júnior, L., & Bru, J. -B. (2019). The discreteness-driven relaxation of collisionless gravitating systems: entropy evolution in external potentials, n-dependence and the role of chaos. The Astrophysical Journal, 870( 2), 128. doi:10.3847/1538-4357/aaf397
NLM
Silva LB e, De Siqueira Pedra W, Valluri M, Sodré Júnior L, Bru J-B. The discreteness-driven relaxation of collisionless gravitating systems: entropy evolution in external potentials, n-dependence and the role of chaos [Internet]. The Astrophysical Journal. 2019 ;870( 2): 128.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/aaf397
Vancouver
Silva LB e, De Siqueira Pedra W, Valluri M, Sodré Júnior L, Bru J-B. The discreteness-driven relaxation of collisionless gravitating systems: entropy evolution in external potentials, n-dependence and the role of chaos [Internet]. The Astrophysical Journal. 2019 ;870( 2): 128.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/aaf397
Artigo de periodico
What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars? (2019)
Guerrero, G; Zaire, B; Smolarkiewicz, P. K; Dal Pino, Elisabete Maria de Gouveia ; Kosovichev, A. G; Mansour, N. N
Source: The Astrophysical Journal. Unidade: IAG
Subjects: CAMPO MAGNÉTICO, ASTROFÍSICA SOLAR
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ABNT
GUERRERO, G et al. What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars?. The Astrophysical Journal, v. 880, n. 1, p. 6/1-6/20, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab224a. Acesso em: 05 nov. 2024.
APA
Guerrero, G., Zaire, B., Smolarkiewicz, P. K., Dal Pino, E. M. de G., Kosovichev, A. G., & Mansour, N. N. (2019). What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars? The Astrophysical Journal, 880( 1), 6/1-6/20. doi:10.3847/1538-4357/ab224a
NLM
Guerrero G, Zaire B, Smolarkiewicz PK, Dal Pino EM de G, Kosovichev AG, Mansour NN. What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars? [Internet]. The Astrophysical Journal. 2019 ; 880( 1): 6/1-6/20.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab224a
Vancouver
Guerrero G, Zaire B, Smolarkiewicz PK, Dal Pino EM de G, Kosovichev AG, Mansour NN. What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars? [Internet]. The Astrophysical Journal. 2019 ; 880( 1): 6/1-6/20.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab224a
Artigo de periodico
Integrated Spectra of Milky Way Globular Clusters (2019)
Moura, T. C; Trevisan, M; Barbuy, Beatriz Leonor Silveira; Rossi, Silvia Cristina Fernandes
Source: The Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), ATMOSFERAS ESTELARES, POPULAÇÕES ESTELARES
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ABNT
MOURA, T. C et al. Integrated Spectra of Milky Way Globular Clusters. The Astrophysical Journal, v. No, n. 1, p. 28/1-28/23, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab3eb6. Acesso em: 05 nov. 2024.
APA
Moura, T. C., Trevisan, M., Barbuy, B. L. S., & Rossi, S. C. F. (2019). Integrated Spectra of Milky Way Globular Clusters. The Astrophysical Journal, No( 1), 28/1-28/23. doi:10.3847/1538-4357/ab3eb6
NLM
Moura TC, Trevisan M, Barbuy BLS, Rossi SCF. Integrated Spectra of Milky Way Globular Clusters [Internet]. The Astrophysical Journal. 2019 ; No( 1): 28/1-28/23.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab3eb6
Vancouver
Moura TC, Trevisan M, Barbuy BLS, Rossi SCF. Integrated Spectra of Milky Way Globular Clusters [Internet]. The Astrophysical Journal. 2019 ; No( 1): 28/1-28/23.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab3eb6
Artigo de periodico
G331.512-0.103: An Interstellar Laboratory for Molecular Synthesis I. The Ortho-to-para Ratios for CH3OH and CH3CN (2018)
Mendoza, Edgar; Bronfman, Leonardo; Duronea, Nicolas U; Lépine, Jacques Raymond Daniel; Finger, Ricardo; Merello, Manuel; Caimapo, Carlos Hervías; Gama, Diana Renata Gonçalves; Ake-Nyman, Lars
Source: The Astrophysical Journal. Unidade: IAG
Assunto: MEIO INTERESTELAR
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ABNT
MENDOZA, Edgar et al. G331.512-0.103: An Interstellar Laboratory for Molecular Synthesis I. The Ortho-to-para Ratios for CH3OH and CH3CN. The Astrophysical Journal, v. 853, p. 152, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aaa1ec. Acesso em: 05 nov. 2024.
APA
Mendoza, E., Bronfman, L., Duronea, N. U., Lépine, J. R. D., Finger, R., Merello, M., et al. (2018). G331.512-0.103: An Interstellar Laboratory for Molecular Synthesis I. The Ortho-to-para Ratios for CH3OH and CH3CN. The Astrophysical Journal, 853, 152. doi:10.3847/1538-4357/aaa1ec
NLM
Mendoza E, Bronfman L, Duronea NU, Lépine JRD, Finger R, Merello M, Caimapo CH, Gama DRG, Ake-Nyman L. G331.512-0.103: An Interstellar Laboratory for Molecular Synthesis I. The Ortho-to-para Ratios for CH3OH and CH3CN [Internet]. The Astrophysical Journal. 2018 ; 853 152.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/aaa1ec
Vancouver
Mendoza E, Bronfman L, Duronea NU, Lépine JRD, Finger R, Merello M, Caimapo CH, Gama DRG, Ake-Nyman L. G331.512-0.103: An Interstellar Laboratory for Molecular Synthesis I. The Ortho-to-para Ratios for CH3OH and CH3CN [Internet]. The Astrophysical Journal. 2018 ; 853 152.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/aaa1ec
Artigo de periodico
NGC 6744: a nearby Milky Way twin with a very low-luminosity AGN (2018)
SILVA, Patricia da; Steiner, João Evangelista; Menezes, R.B
Source: The Astrophysical Journal. Unidade: IAG
Assunto: GALÁXIAS ATIVAS
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ABNT
SILVA, Patricia da e STEINER, João Evangelista e MENEZES, R.B. NGC 6744: a nearby Milky Way twin with a very low-luminosity AGN. The Astrophysical Journal, v. 861, p. 83, 2018Tradução . . Disponível em: https://arxiv.org/pdf/1807.02604.pdf. Acesso em: 05 nov. 2024.
APA
SILVA, P. da, Steiner, J. E., & Menezes, R. B. (2018). NGC 6744: a nearby Milky Way twin with a very low-luminosity AGN. The Astrophysical Journal, 861, 83. doi:10.3847/1538-4357/aac6e3
NLM
SILVA P da, Steiner JE, Menezes RB. NGC 6744: a nearby Milky Way twin with a very low-luminosity AGN [Internet]. The Astrophysical Journal. 2018 ; 861 83.[citado 2024 nov. 05 ] Available from: https://arxiv.org/pdf/1807.02604.pdf
Vancouver
SILVA P da, Steiner JE, Menezes RB. NGC 6744: a nearby Milky Way twin with a very low-luminosity AGN [Internet]. The Astrophysical Journal. 2018 ; 861 83.[citado 2024 nov. 05 ] Available from: https://arxiv.org/pdf/1807.02604.pdf
Artigo de periodico
Erratum: The role of fast magnetic reconnection on the radio and gamma-ray emission from the nuclear regions of microquasars and Low luminosity AGNs (2018)
Kadowaki, L. H. S; Dal Pino, Elisabete Maria de Gouveia; Singh, Chandra B
Source: The Astrophysical Journal. Unidade: IAG
Subjects: DISCOS DE ACRESÇÃO, GALÁXIAS ATIVAS, RAIOS GAMA, MAGNETISMO, ESTRELAS BINÁRIAS
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ABNT
KADOWAKI, L. H. S e DAL PINO, Elisabete Maria de Gouveia e SINGH, Chandra B. Erratum: The role of fast magnetic reconnection on the radio and gamma-ray emission from the nuclear regions of microquasars and Low luminosity AGNs. The Astrophysical Journal, v. 857, p. 146, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aabba8. Acesso em: 05 nov. 2024.
APA
Kadowaki, L. H. S., Dal Pino, E. M. de G., & Singh, C. B. (2018). Erratum: The role of fast magnetic reconnection on the radio and gamma-ray emission from the nuclear regions of microquasars and Low luminosity AGNs. The Astrophysical Journal, 857, 146. doi:10.3847/1538-4357/aabba8
NLM
Kadowaki LHS, Dal Pino EM de G, Singh CB. Erratum: The role of fast magnetic reconnection on the radio and gamma-ray emission from the nuclear regions of microquasars and Low luminosity AGNs [Internet]. The Astrophysical Journal. 2018 ; 857 146.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/aabba8
Vancouver
Kadowaki LHS, Dal Pino EM de G, Singh CB. Erratum: The role of fast magnetic reconnection on the radio and gamma-ray emission from the nuclear regions of microquasars and Low luminosity AGNs [Internet]. The Astrophysical Journal. 2018 ; 857 146.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/aabba8
Artigo de periodico
Spatial growth of current-driven instability in relativistic rotating jets and the search for magnetic reconnection (2016)
Singh, Chandra B; Mizuno, Yosuke; Dal Pino, Elisabete Maria de Gouveia
Source: The Astrophysical Journal. Unidade: IAG
Subjects: JATOS (ASTRONOMIA), GALÁXIAS
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ABNT
SINGH, Chandra B e MIZUNO, Yosuke e DAL PINO, Elisabete Maria de Gouveia. Spatial growth of current-driven instability in relativistic rotating jets and the search for magnetic reconnection. The Astrophysical Journal, 2016Tradução . . Disponível em: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0004-637X/824/1/48/pdf. Acesso em: 05 nov. 2024.
APA
Singh, C. B., Mizuno, Y., & Dal Pino, E. M. de G. (2016). Spatial growth of current-driven instability in relativistic rotating jets and the search for magnetic reconnection. The Astrophysical Journal. doi:10.3847/0004-637X/824/1/48
NLM
Singh CB, Mizuno Y, Dal Pino EM de G. Spatial growth of current-driven instability in relativistic rotating jets and the search for magnetic reconnection [Internet]. The Astrophysical Journal. 2016 ;[citado 2024 nov. 05 ] Available from: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0004-637X/824/1/48/pdf
Vancouver
Singh CB, Mizuno Y, Dal Pino EM de G. Spatial growth of current-driven instability in relativistic rotating jets and the search for magnetic reconnection [Internet]. The Astrophysical Journal. 2016 ;[citado 2024 nov. 05 ] Available from: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0004-637X/824/1/48/pdf
Artigo de periodico
A mid-infrared view of the high mass star formation region W51A (2016)
Barbosa, C. L; Blum, R. D; Damineli Neto, Augusto; Conti, P. S; Gusmão, D. M
Source: The Astrophysical Journal. Unidade: IAG
Subjects: ASTROFÍSICA ESTELAR, INFRAVERMELHO
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ABNT
BARBOSA, C. L et al. A mid-infrared view of the high mass star formation region W51A. The Astrophysical Journal, 2016Tradução . . Disponível em: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0004-637X/825/1/54/pdf. Acesso em: 05 nov. 2024.
APA
Barbosa, C. L., Blum, R. D., Damineli Neto, A., Conti, P. S., & Gusmão, D. M. (2016). A mid-infrared view of the high mass star formation region W51A. The Astrophysical Journal. doi:10.3847/0004-637X/825/1/54
NLM
Barbosa CL, Blum RD, Damineli Neto A, Conti PS, Gusmão DM. A mid-infrared view of the high mass star formation region W51A [Internet]. The Astrophysical Journal. 2016 ;[citado 2024 nov. 05 ] Available from: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0004-637X/825/1/54/pdf
Vancouver
Barbosa CL, Blum RD, Damineli Neto A, Conti PS, Gusmão DM. A mid-infrared view of the high mass star formation region W51A [Internet]. The Astrophysical Journal. 2016 ;[citado 2024 nov. 05 ] Available from: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0004-637X/825/1/54/pdf
Artigo de periodico
He II λ ‘lambda’ 4686 emission from the massive binary system in η ‘eta’car: constraints to the orbital elements and the nature of the periodic minima (2016)
Teodoro, M; Damineli Neto, Augusto; Hickel, G; Henrique, W; Jablonski, F
Source: The Astrophysical Journal. Unidade: IAG
Subjects: ESTRELAS BINÁRIAS, ASTROFÍSICA ESTELAR
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
TEODORO, M et al. He II λ ‘lambda’ 4686 emission from the massive binary system in η ‘eta’car: constraints to the orbital elements and the nature of the periodic minima. The Astrophysical Journal, v. 819, p. 131, 2016Tradução . . Disponível em: http://iopscience.iop.org/article/10.3847/0004-637X/819/2/131/pdf. Acesso em: 05 nov. 2024.
APA
Teodoro, M., Damineli Neto, A., Hickel, G., Henrique, W., & Jablonski, F. (2016). He II λ ‘lambda’ 4686 emission from the massive binary system in η ‘eta’car: constraints to the orbital elements and the nature of the periodic minima. The Astrophysical Journal, 819, 131. doi:10.3847/0004-637X/819/2/131
NLM
Teodoro M, Damineli Neto A, Hickel G, Henrique W, Jablonski F. He II λ ‘lambda’ 4686 emission from the massive binary system in η ‘eta’car: constraints to the orbital elements and the nature of the periodic minima [Internet]. The Astrophysical Journal. 2016 ; 819 131.[citado 2024 nov. 05 ] Available from: http://iopscience.iop.org/article/10.3847/0004-637X/819/2/131/pdf
Vancouver
Teodoro M, Damineli Neto A, Hickel G, Henrique W, Jablonski F. He II λ ‘lambda’ 4686 emission from the massive binary system in η ‘eta’car: constraints to the orbital elements and the nature of the periodic minima [Internet]. The Astrophysical Journal. 2016 ; 819 131.[citado 2024 nov. 05 ] Available from: http://iopscience.iop.org/article/10.3847/0004-637X/819/2/131/pdf
Artigo de periodico
CO observations and investigation of triggered star formation toward the n10 infrared bubble and surroundings (2016)
Gama, Diana Renata Gonçalves; Lépine, Jacques Raymond Daniel; Mendoza, E; Wu, Y; Yuan, J
Source: The Astrophysical Journal. Unidade: IAG
Assunto: ASTROFÍSICA ESTELAR
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
GAMA, Diana Renata Gonçalves et al. CO observations and investigation of triggered star formation toward the n10 infrared bubble and surroundings. The Astrophysical Journal, v. 830, 2016Tradução . . Disponível em: http://iopscience.iop.org/article/10.3847/0004-637X/830/2/57/pdf. Acesso em: 05 nov. 2024.
APA
Gama, D. R. G., Lépine, J. R. D., Mendoza, E., Wu, Y., & Yuan, J. (2016). CO observations and investigation of triggered star formation toward the n10 infrared bubble and surroundings. The Astrophysical Journal, 830. doi:10.3847/0004-637X/830/2/57
NLM
Gama DRG, Lépine JRD, Mendoza E, Wu Y, Yuan J. CO observations and investigation of triggered star formation toward the n10 infrared bubble and surroundings [Internet]. The Astrophysical Journal. 2016 ; 830[citado 2024 nov. 05 ] Available from: http://iopscience.iop.org/article/10.3847/0004-637X/830/2/57/pdf
Vancouver
Gama DRG, Lépine JRD, Mendoza E, Wu Y, Yuan J. CO observations and investigation of triggered star formation toward the n10 infrared bubble and surroundings [Internet]. The Astrophysical Journal. 2016 ; 830[citado 2024 nov. 05 ] Available from: http://iopscience.iop.org/article/10.3847/0004-637X/830/2/57/pdf
Artigo de periodico
A source for point sources of EeV neutrons (2012)
Abreu, P.; Albuquerque, I F M ; Gouffon, P ; Tridapalli, D B
Source: The Astrophysical Journal. Unidade: IF
Assunto: NÊUTRONS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
ABREU, P. et al. A source for point sources of EeV neutrons. The Astrophysical Journal, v. no2012, n. 2, p. 148-159, 2012Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/760/2/148. Acesso em: 05 nov. 2024.
APA
Abreu, P., Albuquerque, I. F. M., Gouffon, P., & Tridapalli, D. B. (2012). A source for point sources of EeV neutrons. The Astrophysical Journal, no2012( 2), 148-159. doi:10.1088/0004-637X/760/2/148
NLM
Abreu P, Albuquerque IFM, Gouffon P, Tridapalli DB. A source for point sources of EeV neutrons [Internet]. The Astrophysical Journal. 2012 ; no2012( 2): 148-159.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1088/0004-637X/760/2/148
Vancouver
Abreu P, Albuquerque IFM, Gouffon P, Tridapalli DB. A source for point sources of EeV neutrons [Internet]. The Astrophysical Journal. 2012 ; no2012( 2): 148-159.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1088/0004-637X/760/2/148

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