ReP USP - Resultado da busca

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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ABNT
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: 11 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. 11 ] 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. 11 ] Available from: https://doi.org/10.3847/1538-4357/ab63ca
Artigo de periodico
Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium (2020)
Jesus, Lorena do Carmo ; González-Casanova, Diego F. ; Falceta Gonçalves, Diego Antonio ; Lazarian, Alex ; Jablonski, Francisco; Zhang, Jian-Fu; Ferreira, Ivan Soares ; Castro, Manuel L. Díaz; Yang, Bo
Source: The Astrophysical Journal. Unidade: EACH
Subjects: MAGNETOHIDRODINÂMICA, MEIO INTERESTELAR
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ABNT
JESUS, Lorena do Carmo et al. Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium. The Astrophysical Journal, v. 905, n. 2, p. 01-12, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/abc331. Acesso em: 11 nov. 2024.
APA
Jesus, L. do C., González-Casanova, D. F., Falceta Gonçalves, D. A., Lazarian, A., Jablonski, F., Zhang, J. -F., et al. (2020). Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium. The Astrophysical Journal, 905( 2), 01-12. doi:10.3847/1538-4357/abc331
NLM
Jesus L do C, González-Casanova DF, Falceta Gonçalves DA, Lazarian A, Jablonski F, Zhang J-F, Ferreira IS, Castro MLD, Yang B. Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium [Internet]. The Astrophysical Journal. 2020 ; 905( 2): 01-12.[citado 2024 nov. 11 ] Available from: https://doi.org/10.3847/1538-4357/abc331
Vancouver
Jesus L do C, González-Casanova DF, Falceta Gonçalves DA, Lazarian A, Jablonski F, Zhang J-F, Ferreira IS, Castro MLD, Yang B. Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium [Internet]. The Astrophysical Journal. 2020 ; 905( 2): 01-12.[citado 2024 nov. 11 ] Available from: https://doi.org/10.3847/1538-4357/abc331
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: 11 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. 11 ] 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. 11 ] Available from: https://doi.org/10.3847/1538-4357/aaa1ec
Artigo de periodico
A new optical polarization catalog for the small Magellanic Cloud: the magnetic field structure (2015)
Gomes, Aiara Lobo; Magalhães, Antônio Mário; Pereyra, Antonio; Rodrigues, Cláudia Vilega
Source: The Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIAS, MEIO INTERESTELAR, NUVENS DE MAGALHÃES, CAMPO MAGNÉTICO
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ABNT
GOMES, Aiara Lobo et al. A new optical polarization catalog for the small Magellanic Cloud: the magnetic field structure. The Astrophysical Journal, v. 806, p. 94/1-94/19, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/806/1/94. Acesso em: 11 nov. 2024.
APA
Gomes, A. L., Magalhães, A. M., Pereyra, A., & Rodrigues, C. V. (2015). A new optical polarization catalog for the small Magellanic Cloud: the magnetic field structure. The Astrophysical Journal, 806, 94/1-94/19. doi:10.1088/0004-637X/806/1/94
NLM
Gomes AL, Magalhães AM, Pereyra A, Rodrigues CV. A new optical polarization catalog for the small Magellanic Cloud: the magnetic field structure [Internet]. The Astrophysical Journal. 2015 ; 806 94/1-94/19.[citado 2024 nov. 11 ] Available from: https://doi.org/10.1088/0004-637X/806/1/94
Vancouver
Gomes AL, Magalhães AM, Pereyra A, Rodrigues CV. A new optical polarization catalog for the small Magellanic Cloud: the magnetic field structure [Internet]. The Astrophysical Journal. 2015 ; 806 94/1-94/19.[citado 2024 nov. 11 ] Available from: https://doi.org/10.1088/0004-637X/806/1/94
Artigo de periodico
Evidence for an interstellar dust filament in the outer heliosheath (2015)
Frisch, P. C; Andersson, B.-G; Berdyugin, A; Piirola, V; Funsten, H. O; Magalhães, Antonio Mário; Seriacopi, D. B; McComas, D. J; Schwadron, N. A; Slavin, J. D; Wiktorowicz, S. J
Source: The Astrophysical Journal. Unidade: IAG
Subjects: POEIRA INTERESTELAR, MEIO INTERESTELAR, CAMPO MAGNÉTICO, POLARIZAÇÃO (ASTRONOMIA), SOL
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ABNT
FRISCH, P. C et al. Evidence for an interstellar dust filament in the outer heliosheath. The Astrophysical Journal, v. 805, p. 60/1-60/8, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/805/1/60. Acesso em: 11 nov. 2024.
APA
Frisch, P. C., Andersson, B. -G., Berdyugin, A., Piirola, V., Funsten, H. O., Magalhães, A. M., et al. (2015). Evidence for an interstellar dust filament in the outer heliosheath. The Astrophysical Journal, 805, 60/1-60/8. doi:10.1088/0004-637X/805/1/60
NLM
Frisch PC, Andersson B-G, Berdyugin A, Piirola V, Funsten HO, Magalhães AM, Seriacopi DB, McComas DJ, Schwadron NA, Slavin JD, Wiktorowicz SJ. Evidence for an interstellar dust filament in the outer heliosheath [Internet]. The Astrophysical Journal. 2015 ; 805 60/1-60/8.[citado 2024 nov. 11 ] Available from: https://doi.org/10.1088/0004-637X/805/1/60
Vancouver
Frisch PC, Andersson B-G, Berdyugin A, Piirola V, Funsten HO, Magalhães AM, Seriacopi DB, McComas DJ, Schwadron NA, Slavin JD, Wiktorowicz SJ. Evidence for an interstellar dust filament in the outer heliosheath [Internet]. The Astrophysical Journal. 2015 ; 805 60/1-60/8.[citado 2024 nov. 11 ] Available from: https://doi.org/10.1088/0004-637X/805/1/60
Artigo de periodico
Magnetic field components analysis of the SCUPOL 850 'mü'm polarization data catalog (2013)
Poidevin, Frédérick; Falceta Gonçalves, Diego Antonio; Kowal, Grzegorz; Dal Pino, Elisabete Maria de Gouveia; Magalhães, Antonio Mário
Source: The Astrophysical Journal. Unidades: IAG, EACH
Subjects: MEIO INTERESTELAR, CAMPO MAGNÉTICO, POLARIZAÇÃO (ASTRONOMIA), TURBULÊNCIA
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ABNT
POIDEVIN, Frédérick et al. Magnetic field components analysis of the SCUPOL 850 'mü'm polarization data catalog. The Astrophysical Journal, v. 777, p. 112/1-112/15, 2013Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/777/2/112. Acesso em: 11 nov. 2024.
APA
Poidevin, F., Falceta Gonçalves, D. A., Kowal, G., Dal Pino, E. M. de G., & Magalhães, A. M. (2013). Magnetic field components analysis of the SCUPOL 850 'mü'm polarization data catalog. The Astrophysical Journal, 777, 112/1-112/15. doi:10.1088/0004-637X/777/2/112
NLM
Poidevin F, Falceta Gonçalves DA, Kowal G, Dal Pino EM de G, Magalhães AM. Magnetic field components analysis of the SCUPOL 850 'mü'm polarization data catalog [Internet]. The Astrophysical Journal. 2013 ; 777 112/1-112/15.[citado 2024 nov. 11 ] Available from: https://doi.org/10.1088/0004-637X/777/2/112
Vancouver
Poidevin F, Falceta Gonçalves DA, Kowal G, Dal Pino EM de G, Magalhães AM. Magnetic field components analysis of the SCUPOL 850 'mü'm polarization data catalog [Internet]. The Astrophysical Journal. 2013 ; 777 112/1-112/15.[citado 2024 nov. 11 ] Available from: https://doi.org/10.1088/0004-637X/777/2/112
Artigo de periodico
The collapse of turbulent cores and reconnection diffusion (2013)
Leão, M. R. M; Dal Pino, Elisabete Maria de Gouveia; Santos-Lima, R; Lazarian, A
Source: The Astrophysical Journal. Unidade: IAG
Subjects: MEIO INTERESTELAR, CAMPO MAGNÉTICO, MAGNETOHIDRODINÂMICA, FORMAÇÃO DE ESTRELAS, TURBULÊNCIA
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ABNT
LEÃO, M. R. M et al. The collapse of turbulent cores and reconnection diffusion. The Astrophysical Journal, v. 777, n. 1, p. 46/1-46/23, 2013Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/777/1/46. Acesso em: 11 nov. 2024.
APA
Leão, M. R. M., Dal Pino, E. M. de G., Santos-Lima, R., & Lazarian, A. (2013). The collapse of turbulent cores and reconnection diffusion. The Astrophysical Journal, 777( 1), 46/1-46/23. doi:10.1088/0004-637X/777/1/46
NLM
Leão MRM, Dal Pino EM de G, Santos-Lima R, Lazarian A. The collapse of turbulent cores and reconnection diffusion [Internet]. The Astrophysical Journal. 2013 ; 777( 1): 46/1-46/23.[citado 2024 nov. 11 ] Available from: https://doi.org/10.1088/0004-637X/777/1/46
Vancouver
Leão MRM, Dal Pino EM de G, Santos-Lima R, Lazarian A. The collapse of turbulent cores and reconnection diffusion [Internet]. The Astrophysical Journal. 2013 ; 777( 1): 46/1-46/23.[citado 2024 nov. 11 ] Available from: https://doi.org/10.1088/0004-637X/777/1/46
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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ABNT
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: 11 nov. 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 nov. 11 ] 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 nov. 11 ] Available from: https://doi.org/10.1088/0004-637X/747/1/21
Artigo de periodico
The compton-thick Seyfert 2 nucleus of NGC 3281: torus constraints from the 9.7 'mü'm silicate absorption (2011)
Sales, Dinalva A; Pastoriza, M. G; Riffel, R; Winge, C; Rodríguez-Ardila, A; Carciofi, Alex Cavaliéri
Source: The Astrophysical Journal. Unidade: IAG
Subjects: INFRAVERMELHO, MEIO INTERESTELAR, GALÁXIAS SEY FERT, ESPECTROSCOPIA, POEIRA INTERESTELAR, GALÁXIAS
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ABNT
SALES, Dinalva A et al. The compton-thick Seyfert 2 nucleus of NGC 3281: torus constraints from the 9.7 'mü'm silicate absorption. The Astrophysical Journal, v. 738, p. 109/1-109/7, 2011Tradução . . Acesso em: 11 nov. 2024.
APA
Sales, D. A., Pastoriza, M. G., Riffel, R., Winge, C., Rodríguez-Ardila, A., & Carciofi, A. C. (2011). The compton-thick Seyfert 2 nucleus of NGC 3281: torus constraints from the 9.7 'mü'm silicate absorption. The Astrophysical Journal, 738, 109/1-109/7.
NLM
Sales DA, Pastoriza MG, Riffel R, Winge C, Rodríguez-Ardila A, Carciofi AC. The compton-thick Seyfert 2 nucleus of NGC 3281: torus constraints from the 9.7 'mü'm silicate absorption. The Astrophysical Journal. 2011 ; 738 109/1-109/7.[citado 2024 nov. 11 ]
Vancouver
Sales DA, Pastoriza MG, Riffel R, Winge C, Rodríguez-Ardila A, Carciofi AC. The compton-thick Seyfert 2 nucleus of NGC 3281: torus constraints from the 9.7 'mü'm silicate absorption. The Astrophysical Journal. 2011 ; 738 109/1-109/7.[citado 2024 nov. 11 ]
Artigo de periodico
Modeling very long baseline interferometric images with the cross-entropy global optmization technique (2011)
Caproni, A; Monteiro, H; Abraham, Zulema; Teixeira, D. M; Toffoli, R. T
Source: The Astrophysical Journal. Unidade: IAG
Subjects: JATOS (ASTRONOMIA), MEIO INTERESTELAR, INTERFEROMETRIA, ANÁLISE DE DADOS, GALÁXIAS
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ABNT
CAPRONI, A et al. Modeling very long baseline interferometric images with the cross-entropy global optmization technique. The Astrophysical Journal, v. 736, p. 68/1-68/18, 2011Tradução . . Acesso em: 11 nov. 2024.
APA
Caproni, A., Monteiro, H., Abraham, Z., Teixeira, D. M., & Toffoli, R. T. (2011). Modeling very long baseline interferometric images with the cross-entropy global optmization technique. The Astrophysical Journal, 736, 68/1-68/18.
NLM
Caproni A, Monteiro H, Abraham Z, Teixeira DM, Toffoli RT. Modeling very long baseline interferometric images with the cross-entropy global optmization technique. The Astrophysical Journal. 2011 ; 736 68/1-68/18.[citado 2024 nov. 11 ]
Vancouver
Caproni A, Monteiro H, Abraham Z, Teixeira DM, Toffoli RT. Modeling very long baseline interferometric images with the cross-entropy global optmization technique. The Astrophysical Journal. 2011 ; 736 68/1-68/18.[citado 2024 nov. 11 ]
Artigo de periodico
Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection (2010)
Santos-Lima, R; Lazarian, A; Dal Pino, Elisabete Maria de Gouveia; Cho, J
Source: The Astrophysical Journal. Unidade: IAG
Subjects: MEIO INTERESTELAR, CAMPO MAGNÉTICO, MAGNETOHIDRODINÂMICA, FORMAÇÃO DE ESTRELAS, TURBULÊNCIA
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ABNT
SANTOS-LIMA, R et al. Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection. The Astrophysical Journal, v. 714, p. 442\2013461, 2010Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/714/1/442. Acesso em: 11 nov. 2024.
APA
Santos-Lima, R., Lazarian, A., Dal Pino, E. M. de G., & Cho, J. (2010). Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection. The Astrophysical Journal, 714, 442\2013461. doi:10.1088/0004-637X/714/1/442
NLM
Santos-Lima R, Lazarian A, Dal Pino EM de G, Cho J. Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection [Internet]. The Astrophysical Journal. 2010 ; 714 442\2013461.[citado 2024 nov. 11 ] Available from: https://doi.org/10.1088/0004-637X/714/1/442
Vancouver
Santos-Lima R, Lazarian A, Dal Pino EM de G, Cho J. Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection [Internet]. The Astrophysical Journal. 2010 ; 714 442\2013461.[citado 2024 nov. 11 ] Available from: https://doi.org/10.1088/0004-637X/714/1/442
Artigo de periodico
On the detemination of the rotational oblateness of achernar (2008)
Carciofi, A. C; Domiciano de Souza, A; Magalhães, Antonio Mário; Bjorkman, J. E; Vakili, F
Source: The Astrophysical Journal. Unidade: IAG
Subjects: MEIO INTERESTELAR, ESTRELAS
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ABNT
CARCIOFI, A. C et al. On the detemination of the rotational oblateness of achernar. The Astrophysical Journal, v. 676, p. L41-L44, 2008Tradução . . Acesso em: 11 nov. 2024.
APA
Carciofi, A. C., Domiciano de Souza, A., Magalhães, A. M., Bjorkman, J. E., & Vakili, F. (2008). On the detemination of the rotational oblateness of achernar. The Astrophysical Journal, 676, L41-L44.
NLM
Carciofi AC, Domiciano de Souza A, Magalhães AM, Bjorkman JE, Vakili F. On the detemination of the rotational oblateness of achernar. The Astrophysical Journal. 2008 ; 676 L41-L44.[citado 2024 nov. 11 ]
Vancouver
Carciofi AC, Domiciano de Souza A, Magalhães AM, Bjorkman JE, Vakili F. On the detemination of the rotational oblateness of achernar. The Astrophysical Journal. 2008 ; 676 L41-L44.[citado 2024 nov. 11 ]

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