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Artigo de periodico
η Carinae baby homunculus uncovered by ALMA (2014)
Abraham, Zulema; Falceta Gonçalves, Diego Antonio; Beaklini, Pedro Paulo Bonetti
Source: The Astrophysical Journal. Unidades: IAG, EACH
Subjects: ESTRELAS BINÁRIAS, PERDA DE MASSA, VENTO, ASTROFÍSICA ESTELAR
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ABRAHAM, Zulema e FALCETA GONÇALVES, Diego Antonio e BEAKLINI, Pedro Paulo Bonetti. η Carinae baby homunculus uncovered by ALMA. The Astrophysical Journal, v. 791, n. 2, p. 1-10, 2014Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/791/2/95. Acesso em: 26 abr. 2024.
APA
Abraham, Z., Falceta Gonçalves, D. A., & Beaklini, P. P. B. (2014). η Carinae baby homunculus uncovered by ALMA. The Astrophysical Journal, 791( 2), 1-10. doi:10.1088/0004-637X/791/2/95
NLM
Abraham Z, Falceta Gonçalves DA, Beaklini PPB. η Carinae baby homunculus uncovered by ALMA [Internet]. The Astrophysical Journal. 2014 ; 791( 2): 1-10.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/791/2/95
Vancouver
Abraham Z, Falceta Gonçalves DA, Beaklini PPB. η Carinae baby homunculus uncovered by ALMA [Internet]. The Astrophysical Journal. 2014 ; 791( 2): 1-10.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/791/2/95
Artigo de periodico
X-ray spectral variation of 'eta'Carinae through the 2003 X-ray minimum (2007)
Hamaguchi, Kenji; Corcoran, Michael F; Gull, Theodore; Ishibashi, Kazunori; Pittard, Julian M; Hillier, D. John; Damineli Neto, Augusto; Davidson, Kris; Nielsen, Krister E; Kober, Gladys Viera
Source: The Astrophysical Journal. Unidade: IAG
Subjects: ESTRELAS BINÁRIAS, RAIOS X, ESTRELAS
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HAMAGUCHI, Kenji et al. X-ray spectral variation of 'eta'Carinae through the 2003 X-ray minimum. The Astrophysical Journal, v. 663, n. 1, p. 522-542, 2007Tradução . . Acesso em: 26 abr. 2024.
APA
Hamaguchi, K., Corcoran, M. F., Gull, T., Ishibashi, K., Pittard, J. M., Hillier, D. J., et al. (2007). X-ray spectral variation of 'eta'Carinae through the 2003 X-ray minimum. The Astrophysical Journal, 663( 1), 522-542.
NLM
Hamaguchi K, Corcoran MF, Gull T, Ishibashi K, Pittard JM, Hillier DJ, Damineli Neto A, Davidson K, Nielsen KE, Kober GV. X-ray spectral variation of 'eta'Carinae through the 2003 X-ray minimum. The Astrophysical Journal. 2007 ;663( 1): 522-542.[citado 2024 abr. 26 ]
Vancouver
Hamaguchi K, Corcoran MF, Gull T, Ishibashi K, Pittard JM, Hillier DJ, Damineli Neto A, Davidson K, Nielsen KE, Kober GV. X-ray spectral variation of 'eta'Carinae through the 2003 X-ray minimum. The Astrophysical Journal. 2007 ;663( 1): 522-542.[citado 2024 abr. 26 ]
Artigo de periodico
X-ray emission from Eta Carinae near periastron in 2009: I. A two-state solution (2014)
Hamaguchi, Kenji; Corcoran, Michael F; Russell, Christopher M. P.; Pollock, A. M. T.; Gull, Theodore R; Teodoro, Mairan; Madura, Thomas I.; Damineli Neto, Augusto; Pittard, Julian M
Source: The Astrophysical Journal. Unidade: IAG
Subjects: ESTRELAS BINÁRIAS, ESTRELAS, RAIOS X
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HAMAGUCHI, Kenji et al. X-ray emission from Eta Carinae near periastron in 2009: I. A two-state solution. The Astrophysical Journal, v. 784, n. 125, p. 1-6, 2014Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/784/2/125. Acesso em: 26 abr. 2024.
APA
Hamaguchi, K., Corcoran, M. F., Russell, C. M. P., Pollock, A. M. T., Gull, T. R., Teodoro, M., et al. (2014). X-ray emission from Eta Carinae near periastron in 2009: I. A two-state solution. The Astrophysical Journal, 784( 125), 1-6. doi:10.1088/0004-637X/784/2/125
NLM
Hamaguchi K, Corcoran MF, Russell CMP, Pollock AMT, Gull TR, Teodoro M, Madura TI, Damineli Neto A, Pittard JM. X-ray emission from Eta Carinae near periastron in 2009: I. A two-state solution [Internet]. The Astrophysical Journal. 2014 ;784( 125): 1-6.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/784/2/125
Vancouver
Hamaguchi K, Corcoran MF, Russell CMP, Pollock AMT, Gull TR, Teodoro M, Madura TI, Damineli Neto A, Pittard JM. X-ray emission from Eta Carinae near periastron in 2009: I. A two-state solution [Internet]. The Astrophysical Journal. 2014 ;784( 125): 1-6.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/784/2/125
Artigo de periodico
X-Ray AGB Stars in the 4XMM-DR9 Catalog: Further Evidence for Companions (2021)
Ortiz, Roberto Pereira ; Guerrero, Martín A
Source: The Astrophysical Journal. Unidade: EACH
Subjects: ESTRELAS BINÁRIAS, RAIOS X, ASTROFÍSICA ESTELAR
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ORTIZ, Roberto Pereira e GUERRERO, Martín A. X-Ray AGB Stars in the 4XMM-DR9 Catalog: Further Evidence for Companions. The Astrophysical Journal, v. 912, n. 2, p. 01-14, 2021Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/abefd7. Acesso em: 26 abr. 2024.
APA
Ortiz, R. P., & Guerrero, M. A. (2021). X-Ray AGB Stars in the 4XMM-DR9 Catalog: Further Evidence for Companions. The Astrophysical Journal, 912( 2), 01-14. doi:10.3847/1538-4357/abefd7
NLM
Ortiz RP, Guerrero MA. X-Ray AGB Stars in the 4XMM-DR9 Catalog: Further Evidence for Companions [Internet]. The Astrophysical Journal. 2021 ; 912( 2): 01-14.[citado 2024 abr. 26 ] Available from: https://doi.org/10.3847/1538-4357/abefd7
Vancouver
Ortiz RP, Guerrero MA. X-Ray AGB Stars in the 4XMM-DR9 Catalog: Further Evidence for Companions [Internet]. The Astrophysical Journal. 2021 ; 912( 2): 01-14.[citado 2024 abr. 26 ] Available from: https://doi.org/10.3847/1538-4357/abefd7
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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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: 26 abr. 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 abr. 26 ] 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 abr. 26 ] Available from: https://doi.org/10.3847/1538-4357/ab224a
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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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: 26 abr. 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 abr. 26 ] 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 abr. 26 ] Available from: https://doi.org/10.3847/1538-4357/ab212e
Artigo de periodico
Ultra-high energy cosmic rays: Are they isotropic? (2001)
Medina Tanco, Gustavo Adolfo
Source: The Astrophysical Journal. Unidade: IAG
Assunto: ASTROFÍSICA ESTELAR
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MEDINA TANCO, Gustavo Adolfo. Ultra-high energy cosmic rays: Are they isotropic?. The Astrophysical Journal, v. 549, p. 711-715, 2001Tradução . . Acesso em: 26 abr. 2024.
APA
Medina Tanco, G. A. (2001). Ultra-high energy cosmic rays: Are they isotropic? The Astrophysical Journal, 549, 711-715.
NLM
Medina Tanco GA. Ultra-high energy cosmic rays: Are they isotropic? The Astrophysical Journal. 2001 ; 549 711-715.[citado 2024 abr. 26 ]
Vancouver
Medina Tanco GA. Ultra-high energy cosmic rays: Are they isotropic? The Astrophysical Journal. 2001 ; 549 711-715.[citado 2024 abr. 26 ]
Artigo de periodico
Toward understanding the B[e] phenomenon: IV. modeling of IRAS 00470+6429 (2010)
Carciofi, Alex Cavaliéri; Miroshnichenko, A. S; Bjorkman, J.E
Source: The Astrophysical Journal. Unidade: IAG
Assunto: ESTRELAS
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CARCIOFI, Alex Cavaliéri e MIROSHNICHENKO, A. S e BJORKMAN, J.E. Toward understanding the B[e] phenomenon: IV. modeling of IRAS 00470+6429. The Astrophysical Journal, v. 721, p. 1079-1089, 2010Tradução . . Acesso em: 26 abr. 2024.
APA
Carciofi, A. C., Miroshnichenko, A. S., & Bjorkman, J. E. (2010). Toward understanding the B[e] phenomenon: IV. modeling of IRAS 00470+6429. The Astrophysical Journal, 721, 1079-1089.
NLM
Carciofi AC, Miroshnichenko AS, Bjorkman JE. Toward understanding the B[e] phenomenon: IV. modeling of IRAS 00470+6429. The Astrophysical Journal. 2010 ; 721 1079-1089.[citado 2024 abr. 26 ]
Vancouver
Carciofi AC, Miroshnichenko AS, Bjorkman JE. Toward understanding the B[e] phenomenon: IV. modeling of IRAS 00470+6429. The Astrophysical Journal. 2010 ; 721 1079-1089.[citado 2024 abr. 26 ]
Artigo de periodico
Toward a better understanding of the GRB phenomenon: a new model for GRB prompt emission and its effects on the new LiNT-- E rest.NT peak, i relation (2015)
Guiriec, S; Kouveliotou, C; Daigne, F; Souza, Rodrigo Nemmen da
Source: The Astrophysical Journal. Unidade: IAG
Subjects: ACELERAÇÃO DE PARTÍCULAS, BURACOS NEGROS, RAIOS GAMA, RADIAÇÃO TÉRMICA, RADIAÇÃO NÃO TÉRMICA
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GUIRIEC, S et al. Toward a better understanding of the GRB phenomenon: a new model for GRB prompt emission and its effects on the new LiNT-- E rest.NT peak, i relation. The Astrophysical Journal, v. 807, p. 148/1-148/55, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/807/2/148. Acesso em: 26 abr. 2024.
APA
Guiriec, S., Kouveliotou, C., Daigne, F., & Souza, R. N. da. (2015). Toward a better understanding of the GRB phenomenon: a new model for GRB prompt emission and its effects on the new LiNT-- E rest.NT peak, i relation. The Astrophysical Journal, 807, 148/1-148/55. doi:10.1088/0004-637X/807/2/148
NLM
Guiriec S, Kouveliotou C, Daigne F, Souza RN da. Toward a better understanding of the GRB phenomenon: a new model for GRB prompt emission and its effects on the new LiNT-- E rest.NT peak, i relation [Internet]. The Astrophysical Journal. 2015 ; 807 148/1-148/55.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/807/2/148
Vancouver
Guiriec S, Kouveliotou C, Daigne F, Souza RN da. Toward a better understanding of the GRB phenomenon: a new model for GRB prompt emission and its effects on the new LiNT-- E rest.NT peak, i relation [Internet]. The Astrophysical Journal. 2015 ; 807 148/1-148/55.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/807/2/148
Artigo de periodico
Three-dimensional numerical simulations of magnetized winds of solar-like stars (2009)
Vidotto, A. A; Opher, M; Pereira,Vera Jatenco; Gombosi, T. I
Source: The Astrophysical Journal. Unidade: IAG
Subjects: MÉTODOS NUMÉRICOS, MAGNETOHIDRODINÂMICA, ESTRELAS, VENTO
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VIDOTTO, A. A et al. Three-dimensional numerical simulations of magnetized winds of solar-like stars. The Astrophysical Journal, v. 699, p. 441-452, 2009Tradução . . Acesso em: 26 abr. 2024.
APA
Vidotto, A. A., Opher, M., Pereira, V. J., & Gombosi, T. I. (2009). Three-dimensional numerical simulations of magnetized winds of solar-like stars. The Astrophysical Journal, 699, 441-452.
NLM
Vidotto AA, Opher M, Pereira VJ, Gombosi TI. Three-dimensional numerical simulations of magnetized winds of solar-like stars. The Astrophysical Journal. 2009 ;699 441-452.[citado 2024 abr. 26 ]
Vancouver
Vidotto AA, Opher M, Pereira VJ, Gombosi TI. Three-dimensional numerical simulations of magnetized winds of solar-like stars. The Astrophysical Journal. 2009 ;699 441-452.[citado 2024 abr. 26 ]
Artigo de periodico
Three-dimensional magnetohydrodynamic simulations of radiatively cooling, pulsed jets (2001)
Cerqueira, Adriano H; Gouveia dal Pino, Elisabete Maria de
Source: The Astrophysical Journal. Unidade: IAG
Assunto: GALÁXIAS
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CERQUEIRA, Adriano H e GOUVEIA DAL PINO, Elisabete Maria de. Three-dimensional magnetohydrodynamic simulations of radiatively cooling, pulsed jets. The Astrophysical Journal, v. 560, p. 779-791, 2001Tradução . . Acesso em: 26 abr. 2024.
APA
Cerqueira, A. H., & Gouveia dal Pino, E. M. de. (2001). Three-dimensional magnetohydrodynamic simulations of radiatively cooling, pulsed jets. The Astrophysical Journal, 560, 779-791.
NLM
Cerqueira AH, Gouveia dal Pino EM de. Three-dimensional magnetohydrodynamic simulations of radiatively cooling, pulsed jets. The Astrophysical Journal. 2001 ; 560 779-791.[citado 2024 abr. 26 ]
Vancouver
Cerqueira AH, Gouveia dal Pino EM de. Three-dimensional magnetohydrodynamic simulations of radiatively cooling, pulsed jets. The Astrophysical Journal. 2001 ; 560 779-791.[citado 2024 abr. 26 ]
Artigo de periodico
Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor (2015)
Caproni, Anderson; Lanfranchi, Gustavo Amaral; Silva, A. Luiz da; Falceta Gonçalves, Diego Antonio
Source: The Astrophysical Journal. Unidade: EACH
Subjects: GALÁXIAS, EVOLUÇÃO ESTELAR, HIDRODINÂMICA
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CAPRONI, Anderson et al. Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor. The Astrophysical Journal, v. 805, n. ju 2015, p. 1-12, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/805/2/109. Acesso em: 26 abr. 2024.
APA
Caproni, A., Lanfranchi, G. A., Silva, A. L. da, & Falceta Gonçalves, D. A. (2015). Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor. The Astrophysical Journal, 805( ju 2015), 1-12. doi:10.1088/0004-637X/805/2/109
NLM
Caproni A, Lanfranchi GA, Silva AL da, Falceta Gonçalves DA. Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor [Internet]. The Astrophysical Journal. 2015 ; 805( ju 2015): 1-12.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/805/2/109
Vancouver
Caproni A, Lanfranchi GA, Silva AL da, Falceta Gonçalves DA. Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor [Internet]. The Astrophysical Journal. 2015 ; 805( ju 2015): 1-12.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/805/2/109
Artigo de periodico
Three-Dimensional photoionization structure ande distances of planetary nebulae. IV. NGC 40 (2011)
Monteiro, Hektor; Falceta Gonçalves, Diego Antonio
Source: The Astrophysical Journal. Unidade: EACH
Subjects: ASTROFÍSICA ESTELAR, NEBULOSAS, MEIO INTERGALÁTICO
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MONTEIRO, Hektor e FALCETA GONÇALVES, Diego Antonio. Three-Dimensional photoionization structure ande distances of planetary nebulae. IV. NGC 40. The Astrophysical Journal, v. 738, n. 2, p. 1-10, 2011Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/738/2/174. Acesso em: 26 abr. 2024.
APA
Monteiro, H., & Falceta Gonçalves, D. A. (2011). Three-Dimensional photoionization structure ande distances of planetary nebulae. IV. NGC 40. The Astrophysical Journal, 738( 2), 1-10. doi:10.1088/0004-637X/738/2/174
NLM
Monteiro H, Falceta Gonçalves DA. Three-Dimensional photoionization structure ande distances of planetary nebulae. IV. NGC 40 [Internet]. The Astrophysical Journal. 2011 ; 738( 2): 1-10.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/738/2/174
Vancouver
Monteiro H, Falceta Gonçalves DA. Three-Dimensional photoionization structure ande distances of planetary nebulae. IV. NGC 40 [Internet]. The Astrophysical Journal. 2011 ; 738( 2): 1-10.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/738/2/174
Artigo de periodico
The viscosity parameters dependence on the profile of the disk scale height (2008)
Meirelles Filho, César; Leister, Nelson Vani
Source: The Astrophysical Journal. Unidade: IAG
Subjects: DISCOS DE ACRESÇÃO, ASTROFÍSICA ESTELAR
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MEIRELLES FILHO, César e LEISTER, Nelson Vani. The viscosity parameters dependence on the profile of the disk scale height. The Astrophysical Journal, v. 672, p. L45-L48, 2008Tradução . . Acesso em: 26 abr. 2024.
APA
Meirelles Filho, C., & Leister, N. V. (2008). The viscosity parameters dependence on the profile of the disk scale height. The Astrophysical Journal, 672, L45-L48.
NLM
Meirelles Filho C, Leister NV. The viscosity parameters dependence on the profile of the disk scale height. The Astrophysical Journal. 2008 ; 672 L45-L48.[citado 2024 abr. 26 ]
Vancouver
Meirelles Filho C, Leister NV. The viscosity parameters dependence on the profile of the disk scale height. The Astrophysical Journal. 2008 ; 672 L45-L48.[citado 2024 abr. 26 ]
Artigo de periodico
The role of turbulent magnetic reconnection in the formation of rotationally supported protostellar disks (2012)
Santos-Lima, R; Dal Pino, Elisabete Maria de Gouveia; Lazarian, A
Source: The Astrophysical Journal. Unidade: IAG
Subjects: DISCOS DE ACRESÇÃO, MEIO INTERESTELAR, CAMPO MAGNÉTICO, MAGNETOHIDRODINÂMICA, FORMAÇÃO DE ESTRELAS, TURBULÊNCIA
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SANTOS-LIMA, R e DAL PINO, Elisabete Maria de Gouveia e LAZARIAN, A. The role of turbulent magnetic reconnection in the formation of rotationally supported protostellar disks. The Astrophysical Journal, v. 747, p. 21/1-21/8, 2012Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/747/1/21. Acesso em: 26 abr. 2024.
APA
Santos-Lima, R., Dal Pino, E. M. de G., & Lazarian, A. (2012). The role of turbulent magnetic reconnection in the formation of rotationally supported protostellar disks. The Astrophysical Journal, 747, 21/1-21/8. doi:10.1088/0004-637X/747/1/21
NLM
Santos-Lima R, Dal Pino EM de G, Lazarian A. The role of turbulent magnetic reconnection in the formation of rotationally supported protostellar disks [Internet]. The Astrophysical Journal. 2012 ; 747 21/1-21/8.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/747/1/21
Vancouver
Santos-Lima R, Dal Pino EM de G, Lazarian A. The role of turbulent magnetic reconnection in the formation of rotationally supported protostellar disks [Internet]. The Astrophysical Journal. 2012 ; 747 21/1-21/8.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/747/1/21
Artigo de periodico
The role of fast magnetic reconnection on the radio and gamma-ray emission from the nuclear regions of microquasars and low luminosity AGNs (2015)
Kadowaki, L. H. S; Dal Pino, Elisabete Maria de Gouveia; Singh, C. B
Source: The Astrophysical Journal. Unidade: IAG
Subjects: DISCOS DE ACRESÇÃO, GALÁXIAS ATIVAS, RAIOS GAMA, MAGNETISMO, ESTRELAS BINÁRIAS
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KADOWAKI, L. H. S e DAL PINO, Elisabete Maria de Gouveia e SINGH, C. B. 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. 802, p. 113/1-113/20, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/802/2/113. Acesso em: 26 abr. 2024.
APA
Kadowaki, L. H. S., Dal Pino, E. M. de G., & Singh, C. B. (2015). 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, 802, 113/1-113/20. doi:10.1088/0004-637X/802/2/113
NLM
Kadowaki LHS, Dal Pino EM de G, Singh CB. 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. 2015 ; 802 113/1-113/20.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/802/2/113
Vancouver
Kadowaki LHS, Dal Pino EM de G, Singh CB. 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. 2015 ; 802 113/1-113/20.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/802/2/113
Artigo de periodico
The quasi-roche lobe overflow state in the evolution of close binary systems containing a radio pulsar (2015)
Benvenuto, O. G; De Vito, M. A; Horvath, Jorge Ernesto
Source: The Astrophysical Journal. Unidade: IAG
Subjects: ESTRELAS, ESTRELAS BINÁRIAS, PULSARES, EVOLUÇÃO ESTELAR
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
BENVENUTO, O. G e DE VITO, M. A e HORVATH, Jorge Ernesto. The quasi-roche lobe overflow state in the evolution of close binary systems containing a radio pulsar. The Astrophysical Journal, v. 798, p. 44/1-44/8, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/798/1/44. Acesso em: 26 abr. 2024.
APA
Benvenuto, O. G., De Vito, M. A., & Horvath, J. E. (2015). The quasi-roche lobe overflow state in the evolution of close binary systems containing a radio pulsar. The Astrophysical Journal, 798, 44/1-44/8. doi:10.1088/0004-637X/798/1/44
NLM
Benvenuto OG, De Vito MA, Horvath JE. The quasi-roche lobe overflow state in the evolution of close binary systems containing a radio pulsar [Internet]. The Astrophysical Journal. 2015 ; 798 44/1-44/8.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/798/1/44
Vancouver
Benvenuto OG, De Vito MA, Horvath JE. The quasi-roche lobe overflow state in the evolution of close binary systems containing a radio pulsar [Internet]. The Astrophysical Journal. 2015 ; 798 44/1-44/8.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/798/1/44
Artigo de periodico
The molecular H2 emission and the stellar kinematics in the nuclear region of the Sombrero galaxy (2015)
Menezes, R. B; Steiner, João Evangelista
Source: The Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIAS ATIVAS, DINÂMICA DAS GALÁXIAS, ESPECTROSCOPIA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
MENEZES, R. B e STEINER, João Evangelista. The molecular H2 emission and the stellar kinematics in the nuclear region of the Sombrero galaxy. The Astrophysical Journal, v. 27, p. 27/1-27/1, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/808/1/27. Acesso em: 26 abr. 2024.
APA
Menezes, R. B., & Steiner, J. E. (2015). The molecular H2 emission and the stellar kinematics in the nuclear region of the Sombrero galaxy. The Astrophysical Journal, 27, 27/1-27/1. doi:10.1088/0004-637X/808/1/27
NLM
Menezes RB, Steiner JE. The molecular H2 emission and the stellar kinematics in the nuclear region of the Sombrero galaxy [Internet]. The Astrophysical Journal. 2015 ; 27 27/1-27/1.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/808/1/27
Vancouver
Menezes RB, Steiner JE. The molecular H2 emission and the stellar kinematics in the nuclear region of the Sombrero galaxy [Internet]. The Astrophysical Journal. 2015 ; 27 27/1-27/1.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/808/1/27
Artigo de periodico
The infrared colors of the sun (2012)
Casagrande, L; Ramírez, I; Meléndez Moreno, Jorge Luis; Asplund, M
Source: The Astrophysical Journal. Unidade: IAG
Subjects: ESTRELAS, SOL, FOTOMETRIA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
CASAGRANDE, L et al. The infrared colors of the sun. The Astrophysical Journal, v. 761, p. 16/1-16/9, 2012Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/761/1/16. Acesso em: 26 abr. 2024.
APA
Casagrande, L., Ramírez, I., Meléndez Moreno, J. L., & Asplund, M. (2012). The infrared colors of the sun. The Astrophysical Journal, 761, 16/1-16/9. doi:10.1088/0004-637X/761/1/16
NLM
Casagrande L, Ramírez I, Meléndez Moreno JL, Asplund M. The infrared colors of the sun [Internet]. The Astrophysical Journal. 2012 ; 761 16/1-16/9.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/761/1/16
Vancouver
Casagrande L, Ramírez I, Meléndez Moreno JL, Asplund M. The infrared colors of the sun [Internet]. The Astrophysical Journal. 2012 ; 761 16/1-16/9.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/761/1/16
Artigo de periodico
The frequency of field blue-straggler stars in the thick disk and halo system of the Galaxy (2015)
Santucci, Rafael M; Placco, Vinicius M; Rossi, Silvia Cristina Fernandes; Beers, Timothy C; Reggiani, Henrique M; Lee, Young Sun; Xue, Xiang-Xiang; Carollo, Daniela
Source: The Astrophysical Journal. Unidade: IAG
Subjects: ESTRELAS BINÁRIAS, ESTRELAS, GALÁXIA (VIA LÁCTEA)
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
SANTUCCI, Rafael M et al. The frequency of field blue-straggler stars in the thick disk and halo system of the Galaxy. The Astrophysical Journal, v. 801, p. 116/1-116/13, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/801/2/116. Acesso em: 26 abr. 2024.
APA
Santucci, R. M., Placco, V. M., Rossi, S. C. F., Beers, T. C., Reggiani, H. M., Lee, Y. S., et al. (2015). The frequency of field blue-straggler stars in the thick disk and halo system of the Galaxy. The Astrophysical Journal, 801, 116/1-116/13. doi:10.1088/0004-637X/801/2/116
NLM
Santucci RM, Placco VM, Rossi SCF, Beers TC, Reggiani HM, Lee YS, Xue X-X, Carollo D. The frequency of field blue-straggler stars in the thick disk and halo system of the Galaxy [Internet]. The Astrophysical Journal. 2015 ; 801 116/1-116/13.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/801/2/116
Vancouver
Santucci RM, Placco VM, Rossi SCF, Beers TC, Reggiani HM, Lee YS, Xue X-X, Carollo D. The frequency of field blue-straggler stars in the thick disk and halo system of the Galaxy [Internet]. The Astrophysical Journal. 2015 ; 801 116/1-116/13.[citado 2024 abr. 26 ] Available from: https://doi.org/10.1088/0004-637X/801/2/116

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