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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: 25 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. 25 ] 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. 25 ] 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: 25 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. 25 ]
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. 25 ]
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: 25 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. 25 ] 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. 25 ] Available from: https://doi.org/10.1088/0004-637X/784/2/125
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: 25 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. 25 ] 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. 25 ] 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: 25 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. 25 ] 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. 25 ] 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: 25 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. 25 ]
Vancouver
Medina Tanco GA. Ultra-high energy cosmic rays: Are they isotropic? The Astrophysical Journal. 2001 ; 549 711-715.[citado 2024 abr. 25 ]
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: 25 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. 25 ]
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. 25 ]
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: 25 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. 25 ] 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. 25 ] 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: 25 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. 25 ]
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. 25 ]
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: 25 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. 25 ]
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. 25 ]
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: 25 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. 25 ]
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. 25 ]
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: 25 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. 25 ] 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. 25 ] 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: 25 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. 25 ] 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. 25 ] 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
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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: 25 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. 25 ] 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. 25 ] 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
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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: 25 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. 25 ] 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. 25 ] 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
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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: 25 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. 25 ] 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. 25 ] 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)
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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: 25 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. 25 ] 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. 25 ] Available from: https://doi.org/10.1088/0004-637X/801/2/116
Artigo de periodico
The distance to SN 1999em from the expanding photosphere method (2001)
Hamuy, Mario; Pinto, Philip A; Maza, José; Suntzeff, Nicholas B; Philips, M M; Eastman, Ronald G; Smith, R C; Corbally, C J; Burstein, D; Li, Yong; Ivanov, Valentin; Moro-Martin, Amaya; Strolger, L G; Souza, R E; Anjos, Sandra dos; Green, Elizabeth M; Pickering, T E; Gonzáles, Luis; Antezana, Roberto; Wischnjewsky, Marina; Galaz, G; Roth, M; Persson, S E; Schommer, R A
Source: The Astrophysical Journal. Unidade: IAG
Assunto: GALÁXIAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
HAMUY, Mario et al. The distance to SN 1999em from the expanding photosphere method. The Astrophysical Journal, v. 558, p. 615-642, 2001Tradução . . Acesso em: 25 abr. 2024.
APA
Hamuy, M., Pinto, P. A., Maza, J., Suntzeff, N. B., Philips, M. M., Eastman, R. G., et al. (2001). The distance to SN 1999em from the expanding photosphere method. The Astrophysical Journal, 558, 615-642.
NLM
Hamuy M, Pinto PA, Maza J, Suntzeff NB, Philips MM, Eastman RG, Smith RC, Corbally CJ, Burstein D, Li Y, Ivanov V, Moro-Martin A, Strolger LG, Souza RE, Anjos S dos, Green EM, Pickering TE, Gonzáles L, Antezana R, Wischnjewsky M, Galaz G, Roth M, Persson SE, Schommer RA. The distance to SN 1999em from the expanding photosphere method. The Astrophysical Journal. 2001 ; 558 615-642.[citado 2024 abr. 25 ]
Vancouver
Hamuy M, Pinto PA, Maza J, Suntzeff NB, Philips MM, Eastman RG, Smith RC, Corbally CJ, Burstein D, Li Y, Ivanov V, Moro-Martin A, Strolger LG, Souza RE, Anjos S dos, Green EM, Pickering TE, Gonzáles L, Antezana R, Wischnjewsky M, Galaz G, Roth M, Persson SE, Schommer RA. The distance to SN 1999em from the expanding photosphere method. The Astrophysical Journal. 2001 ; 558 615-642.[citado 2024 abr. 25 ]
Artigo de periodico
The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system (2015)
Ramírez, I; Khanal, S; Aleo, P; Sobotka, A; Liu, F; Casagrande, L; Moreno, Jorge Luiz Meléndez; Yong, D; Lambert, D. L; Asplund, M
Source: The Astrophysical Journal. Unidade: IAG
Subjects: PLANETAS, ABUNDÂNCIA ESTELAR, ESTRELAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
RAMÍREZ, I et al. The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system. The Astrophysical Journal, v. 808, p. 13/1-13/14, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/808/1/13. Acesso em: 25 abr. 2024.
APA
Ramírez, I., Khanal, S., Aleo, P., Sobotka, A., Liu, F., Casagrande, L., et al. (2015). The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system. The Astrophysical Journal, 808, 13/1-13/14. doi:10.1088/0004-637X/808/1/13
NLM
Ramírez I, Khanal S, Aleo P, Sobotka A, Liu F, Casagrande L, Moreno JLM, Yong D, Lambert DL, Asplund M. The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system [Internet]. The Astrophysical Journal. 2015 ; 808 13/1-13/14.[citado 2024 abr. 25 ] Available from: https://doi.org/10.1088/0004-637X/808/1/13
Vancouver
Ramírez I, Khanal S, Aleo P, Sobotka A, Liu F, Casagrande L, Moreno JLM, Yong D, Lambert DL, Asplund M. The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system [Internet]. The Astrophysical Journal. 2015 ; 808 13/1-13/14.[citado 2024 abr. 25 ] Available from: https://doi.org/10.1088/0004-637X/808/1/13
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; Pedra, Walter Alberto de Siqueira; Valluri, Monica; Sodré Júnior, Laerte; Bru, Jean-Bernard
Source: The Astrophysical Journal. Unidades: IAG, IF
Subjects: GALÁXIAS, MECÂNICA QUÂNTICA, MATEMÁTICA APLICADA, COSMOLOGIA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 25 abr. 2024.
APA
Silva, L. B. e, Pedra, W. A. de S., 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, Pedra WA de S, 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 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/aaf397
Vancouver
Silva LB e, Pedra WA de S, 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 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/aaf397

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