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Trabalho de evento
Non-radial pulsations in the CoRoT Be Star 102761769 (2011)
Janot Pacheco, Eduardo; Andrade, Laerte B. P. de; Emílio, Marcelo; Suárez, Juan Carlos; Jendreieck, Andressa
Fonte: Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESTRELAS, ASTROFÍSICA ESTELAR
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ABNT
JANOT PACHECO, Eduardo et al. Non-radial pulsations in the CoRoT Be Star 102761769. 2011, Anais.. Paris: International Astronomical Union, 2011. . Acesso em: 02 ago. 2024.
APA
Janot Pacheco, E., Andrade, L. B. P. de, Emílio, M., Suárez, J. C., & Jendreieck, A. (2011). Non-radial pulsations in the CoRoT Be Star 102761769. In Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Paris: International Astronomical Union.
NLM
Janot Pacheco E, Andrade LBP de, Emílio M, Suárez JC, Jendreieck A. Non-radial pulsations in the CoRoT Be Star 102761769. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2024 ago. 02 ]
Vancouver
Janot Pacheco E, Andrade LBP de, Emílio M, Suárez JC, Jendreieck A. Non-radial pulsations in the CoRoT Be Star 102761769. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2024 ago. 02 ]
Trabalho de evento-resumo
Kenematic age determinations of planetary nebula central stars (2011)
Rodrigues, T. S; Maciel, Walter Junqueira
Fonte: Planetary nebulae: an eye to the future: Programme & abstracts. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESTRELAS, NEBULOSAS, PLANETAS, MEIO INTERESTELAR
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ABNT
RODRIGUES, T. S e MACIEL, Walter Junqueira. Kenematic age determinations of planetary nebula central stars. 2011, Anais.. Paris: International Astronomical Union, 2011. . Acesso em: 02 ago. 2024.
APA
Rodrigues, T. S., & Maciel, W. J. (2011). Kenematic age determinations of planetary nebula central stars. In Planetary nebulae: an eye to the future: Programme & abstracts. Paris: International Astronomical Union.
NLM
Rodrigues TS, Maciel WJ. Kenematic age determinations of planetary nebula central stars. Planetary nebulae: an eye to the future: Programme & abstracts. 2011 ;[citado 2024 ago. 02 ]
Vancouver
Rodrigues TS, Maciel WJ. Kenematic age determinations of planetary nebula central stars. Planetary nebulae: an eye to the future: Programme & abstracts. 2011 ;[citado 2024 ago. 02 ]
Trabalho de evento
Discussion: Normal and active OB stars as extreme condition test beds (2011)
Gagné, Marc; Janot-Pacheco, Eduardo
Fonte: Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESTRELAS, ASTROFÍSICA ESTELAR
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ABNT
GAGNÉ, Marc e JANOT-PACHECO, Eduardo. Discussion: Normal and active OB stars as extreme condition test beds. 2011, Anais.. Paris: International Astronomical Union, 2011. Disponível em: https://doi.org/10.1017/S1743921311011483. Acesso em: 02 ago. 2024.
APA
Gagné, M., & Janot-Pacheco, E. (2011). Discussion: Normal and active OB stars as extreme condition test beds. In Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Paris: International Astronomical Union. doi:10.1017/S1743921311011483
NLM
Gagné M, Janot-Pacheco E. Discussion: Normal and active OB stars as extreme condition test beds [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311011483
Vancouver
Gagné M, Janot-Pacheco E. Discussion: Normal and active OB stars as extreme condition test beds [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311011483
Trabalho de evento
The dynamical evolution of Be star disks (2011)
Haubois, Xavier; Carciofi, Alex Cavalieri; Okazaki, Atsuo T; Bjorkman, Jon E
Fonte: Active OB stars : structure, evolution, mass loss, and critical limits: proceedings. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: TRANSFERÊNCIA RADIATIVA, ESTRELAS, EVOLUÇÃO ESTELAR
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ABNT
HAUBOIS, Xavier et al. The dynamical evolution of Be star disks. 2011, Anais.. Paris: International Astronomical Union, 2011. . Acesso em: 02 ago. 2024.
APA
Haubois, X., Carciofi, A. C., Okazaki, A. T., & Bjorkman, J. E. (2011). The dynamical evolution of Be star disks. In Active OB stars : structure, evolution, mass loss, and critical limits: proceedings. Paris: International Astronomical Union.
NLM
Haubois X, Carciofi AC, Okazaki AT, Bjorkman JE. The dynamical evolution of Be star disks. Active OB stars : structure, evolution, mass loss, and critical limits: proceedings. 2011 ;[citado 2024 ago. 02 ]
Vancouver
Haubois X, Carciofi AC, Okazaki AT, Bjorkman JE. The dynamical evolution of Be star disks. Active OB stars : structure, evolution, mass loss, and critical limits: proceedings. 2011 ;[citado 2024 ago. 02 ]
Trabalho de evento
The star formation rate in Milky Way: results from stars and planetary nebulae (2011)
Maciel, Walter Junqueira; Rocha-Pinto, H. J.; Costa, Roberto Dell'Aglio Dias da
Fonte: The spectral energy distribution of galaxies (SED 2011): Abstracts. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: FORMAÇÃO DE ESTRELAS, GALÁXIA (VIA LÁCTEA)
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ABNT
MACIEL, Walter Junqueira e ROCHA-PINTO, H. J. e COSTA, Roberto Dell'Aglio Dias da. The star formation rate in Milky Way: results from stars and planetary nebulae. 2011, Anais.. Paris: International Astronomical Union, 2011. . Acesso em: 02 ago. 2024.
APA
Maciel, W. J., Rocha-Pinto, H. J., & Costa, R. D. 'A. D. da. (2011). The star formation rate in Milky Way: results from stars and planetary nebulae. In The spectral energy distribution of galaxies (SED 2011): Abstracts. Paris: International Astronomical Union.
NLM
Maciel WJ, Rocha-Pinto HJ, Costa RD'AD da. The star formation rate in Milky Way: results from stars and planetary nebulae. The spectral energy distribution of galaxies (SED 2011): Abstracts. 2011 ;[citado 2024 ago. 02 ]
Vancouver
Maciel WJ, Rocha-Pinto HJ, Costa RD'AD da. The star formation rate in Milky Way: results from stars and planetary nebulae. The spectral energy distribution of galaxies (SED 2011): Abstracts. 2011 ;[citado 2024 ago. 02 ]
Trabalho de evento
η Carinae long-term variability (2011)
Damineli Neto, Augusto; Teodoro, Mairan; Corcoran, Michael F; Groh, Jose H
Fonte: Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESTRELAS, ESTRELAS VARIÁVEIS, ESTRELAS BINÁRIAS
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ABNT
DAMINELI NETO, Augusto et al. η Carinae long-term variability. 2011, Anais.. Paris: International Astronomical Union, 2011. Disponível em: https://doi.org/10.1017/S1743921311011513. Acesso em: 02 ago. 2024.
APA
Damineli Neto, A., Teodoro, M., Corcoran, M. F., & Groh, J. H. (2011). η Carinae long-term variability. In Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Paris: International Astronomical Union. doi:10.1017/S1743921311011513
NLM
Damineli Neto A, Teodoro M, Corcoran MF, Groh JH. η Carinae long-term variability [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311011513
Vancouver
Damineli Neto A, Teodoro M, Corcoran MF, Groh JH. η Carinae long-term variability [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311011513
Trabalho de evento
Dynamo in the Intra-Cluster Medium: simulation of CGL-MHD turbulent dynamo (2011)
Santos-Lima, R; Gouveia dal Pino, Elisabete Maria de; Lazarian, A.; Kowal, G.; Falceta Gonçalves, Diego Antonio
Fonte: Advances in plasma astrophysics: Proceedings. Nome do evento: IAU Symposium. Unidades: IAG, EACH
Assuntos: CAMPO MAGNÉTICO, MEIO INTERGALÁTICO, PLASMA, MAGNETOHIDRODINÂMICA
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ABNT
SANTOS-LIMA, R et al. Dynamo in the Intra-Cluster Medium: simulation of CGL-MHD turbulent dynamo. 2011, Anais.. Paris: International Astronomical Union, 2011. Disponível em: https://doi.org/10.1017/S1743921311007563. Acesso em: 02 ago. 2024.
APA
Santos-Lima, R., Gouveia dal Pino, E. M. de, Lazarian, A., Kowal, G., & Falceta Gonçalves, D. A. (2011). Dynamo in the Intra-Cluster Medium: simulation of CGL-MHD turbulent dynamo. In Advances in plasma astrophysics: Proceedings. Paris: International Astronomical Union. doi:10.1017/S1743921311007563
NLM
Santos-Lima R, Gouveia dal Pino EM de, Lazarian A, Kowal G, Falceta Gonçalves DA. Dynamo in the Intra-Cluster Medium: simulation of CGL-MHD turbulent dynamo [Internet]. Advances in plasma astrophysics: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311007563
Vancouver
Santos-Lima R, Gouveia dal Pino EM de, Lazarian A, Kowal G, Falceta Gonçalves DA. Dynamo in the Intra-Cluster Medium: simulation of CGL-MHD turbulent dynamo [Internet]. Advances in plasma astrophysics: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311007563
Trabalho de evento
Disk-loss and disk-renewal phases in classical Be stars: II. Detailed analysis of Spectropolarimetric data (2011)
Draper, Zachary H.; Wisniewski, John P; Bjorkman, Karen S.; Bjorkman, Jon E.; Haubois, Xavier; Carciofi, Alex Cavaliéri; Meade, Marilyn R.
Fonte: Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESTRELAS, POLARIZAÇÃO (ASTRONOMIA)
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ABNT
DRAPER, Zachary H. et al. Disk-loss and disk-renewal phases in classical Be stars: II. Detailed analysis of Spectropolarimetric data. 2011, Anais.. Paris: International Astronomical Union, 2011. Disponível em: https://doi.org/10.1017/S1743921311010854. Acesso em: 02 ago. 2024.
APA
Draper, Z. H., Wisniewski, J. P., Bjorkman, K. S., Bjorkman, J. E., Haubois, X., Carciofi, A. C., & Meade, M. R. (2011). Disk-loss and disk-renewal phases in classical Be stars: II. Detailed analysis of Spectropolarimetric data. In Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Paris: International Astronomical Union. doi:10.1017/S1743921311010854
NLM
Draper ZH, Wisniewski JP, Bjorkman KS, Bjorkman JE, Haubois X, Carciofi AC, Meade MR. Disk-loss and disk-renewal phases in classical Be stars: II. Detailed analysis of Spectropolarimetric data [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311010854
Vancouver
Draper ZH, Wisniewski JP, Bjorkman KS, Bjorkman JE, Haubois X, Carciofi AC, Meade MR. Disk-loss and disk-renewal phases in classical Be stars: II. Detailed analysis of Spectropolarimetric data [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311010854
Trabalho de evento
The circumstellar environment of the FS CMa star IRAS 00470+6429 (2011)
Carciofi, Alex Cavaliéri; Miroshnichenko, Anatoly S; Bjorkman, Jon E.
Fonte: Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESTRELAS, VENTO, POEIRA INTERESTELAR
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ABNT
CARCIOFI, Alex Cavaliéri e MIROSHNICHENKO, Anatoly S e BJORKMAN, Jon E. The circumstellar environment of the FS CMa star IRAS 00470+6429. 2011, Anais.. Paris: International Astronomical Union, 2011. Disponível em: https://doi.org/10.1017/S1743921311010830. Acesso em: 02 ago. 2024.
APA
Carciofi, A. C., Miroshnichenko, A. S., & Bjorkman, J. E. (2011). The circumstellar environment of the FS CMa star IRAS 00470+6429. In Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Paris: International Astronomical Union. doi:10.1017/S1743921311010830
NLM
Carciofi AC, Miroshnichenko AS, Bjorkman JE. The circumstellar environment of the FS CMa star IRAS 00470+6429 [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311010830
Vancouver
Carciofi AC, Miroshnichenko AS, Bjorkman JE. The circumstellar environment of the FS CMa star IRAS 00470+6429 [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311010830
Trabalho de evento
Spectrally and spatially resolved Hα emission from Be stars: their disks rotate Keplerian (2011)
Oudmaijer, René D.; Wheelwright, Hugh E.; Carciofi, Alex Cavaliéri; Bjorkman, Jon E; Bjorkman, Karen S
Fonte: Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESTRELAS, ESPECTROS, ASTROFÍSICA ESTELAR
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ABNT
OUDMAIJER, René D. et al. Spectrally and spatially resolved Hα emission from Be stars: their disks rotate Keplerian. 2011, Anais.. Paris: International Astronomical Union, 2011. Disponível em: https://doi.org/10.1017/S1743921311011008. Acesso em: 02 ago. 2024.
APA
Oudmaijer, R. D., Wheelwright, H. E., Carciofi, A. C., Bjorkman, J. E., & Bjorkman, K. S. (2011). Spectrally and spatially resolved Hα emission from Be stars: their disks rotate Keplerian. In Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Paris: International Astronomical Union. doi:10.1017/S1743921311011008
NLM
Oudmaijer RD, Wheelwright HE, Carciofi AC, Bjorkman JE, Bjorkman KS. Spectrally and spatially resolved Hα emission from Be stars: their disks rotate Keplerian [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311011008
Vancouver
Oudmaijer RD, Wheelwright HE, Carciofi AC, Bjorkman JE, Bjorkman KS. Spectrally and spatially resolved Hα emission from Be stars: their disks rotate Keplerian [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311011008
Trabalho de evento
Do cataclysmic variables produce jets? (2011)
Tovmassian, G; Gänsicke, B; Zharikov, S; Ramírez, A; Diaz, Marcos Perez
Fonte: Jets at all scales: Proceedings. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESTRELAS BINÁRIAS, ESPECTROSCOPIA, ESTRELAS NOVAS
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ABNT
TOVMASSIAN, G et al. Do cataclysmic variables produce jets? 2011, Anais.. Paris: International Astronomical Union, 2011. . Acesso em: 02 ago. 2024.
APA
Tovmassian, G., Gänsicke, B., Zharikov, S., Ramírez, A., & Diaz, M. P. (2011). Do cataclysmic variables produce jets? In Jets at all scales: Proceedings. Paris: International Astronomical Union.
NLM
Tovmassian G, Gänsicke B, Zharikov S, Ramírez A, Diaz MP. Do cataclysmic variables produce jets? Jets at all scales: Proceedings. 2011 ;[citado 2024 ago. 02 ]
Vancouver
Tovmassian G, Gänsicke B, Zharikov S, Ramírez A, Diaz MP. Do cataclysmic variables produce jets? Jets at all scales: Proceedings. 2011 ;[citado 2024 ago. 02 ]
Trabalho de evento-resumo
Grids of synthetic spectra for H-poor central stars of planetary nebulae (CSPNe) (2011)
Keller, G. R; Bianchi, L; Herlad, J. E; Maciel, Walter Junqueira
Fonte: Planetary nebulae: an eye to the future: Programme & abstracts. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: PLANETAS, NEBULOSAS
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ABNT
KELLER, G. R et al. Grids of synthetic spectra for H-poor central stars of planetary nebulae (CSPNe). 2011, Anais.. Paris: International Astronomical Union, 2011. . Acesso em: 02 ago. 2024.
APA
Keller, G. R., Bianchi, L., Herlad, J. E., & Maciel, W. J. (2011). Grids of synthetic spectra for H-poor central stars of planetary nebulae (CSPNe). In Planetary nebulae: an eye to the future: Programme & abstracts. Paris: International Astronomical Union.
NLM
Keller GR, Bianchi L, Herlad JE, Maciel WJ. Grids of synthetic spectra for H-poor central stars of planetary nebulae (CSPNe). Planetary nebulae: an eye to the future: Programme & abstracts. 2011 ;[citado 2024 ago. 02 ]
Vancouver
Keller GR, Bianchi L, Herlad JE, Maciel WJ. Grids of synthetic spectra for H-poor central stars of planetary nebulae (CSPNe). Planetary nebulae: an eye to the future: Programme & abstracts. 2011 ;[citado 2024 ago. 02 ]
Trabalho de evento
The Bardeen-Petterson effect as the precession mechanism for the radio galaxy 3C 84 (NGC 1275) (2011)
Teixeira, D. M.; Abraham, Zulema; Caproni, A; Falceta Gonçalves, Diego Antonio
Fonte: Jets at all scales: Proceedings. Nome do evento: IAU Symposium. Unidades: IAG, EACH
Assuntos: GALÁXIAS, JATOS (ASTRONOMIA), DISCOS DE ACRESÇÂO
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ABNT
TEIXEIRA, D. M. et al. The Bardeen-Petterson effect as the precession mechanism for the radio galaxy 3C 84 (NGC 1275). 2011, Anais.. Paris: International Astronomical Union, 2011. Disponível em: https://doi.org/10.1017/S1743921310015954. Acesso em: 02 ago. 2024.
APA
Teixeira, D. M., Abraham, Z., Caproni, A., & Falceta Gonçalves, D. A. (2011). The Bardeen-Petterson effect as the precession mechanism for the radio galaxy 3C 84 (NGC 1275). In Jets at all scales: Proceedings. Paris: International Astronomical Union. doi:10.1017/S1743921310015954
NLM
Teixeira DM, Abraham Z, Caproni A, Falceta Gonçalves DA. The Bardeen-Petterson effect as the precession mechanism for the radio galaxy 3C 84 (NGC 1275) [Internet]. Jets at all scales: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921310015954
Vancouver
Teixeira DM, Abraham Z, Caproni A, Falceta Gonçalves DA. The Bardeen-Petterson effect as the precession mechanism for the radio galaxy 3C 84 (NGC 1275) [Internet]. Jets at all scales: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921310015954
Trabalho de evento-resumo
Planetary nebulae and the chemical evolution of the galactic bulge: new abundances of older objects (2011)
Cavichia, O; Costa, Roberto Dell'Aglio Dias da; Molla, M; Maciel, Walter Junqueira
Fonte: Planetary nebulae: an eye to the future: Programme & abstracts. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: FORMAÇÃO E EVOLUÇÃO DA GALÁXIA, NEBULOSAS
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ABNT
CAVICHIA, O et al. Planetary nebulae and the chemical evolution of the galactic bulge: new abundances of older objects. 2011, Anais.. Paris: International Astronomical Union, 2011. . Acesso em: 02 ago. 2024.
APA
Cavichia, O., Costa, R. D. 'A. D. da, Molla, M., & Maciel, W. J. (2011). Planetary nebulae and the chemical evolution of the galactic bulge: new abundances of older objects. In Planetary nebulae: an eye to the future: Programme & abstracts. Paris: International Astronomical Union.
NLM
Cavichia O, Costa RD'AD da, Molla M, Maciel WJ. Planetary nebulae and the chemical evolution of the galactic bulge: new abundances of older objects. Planetary nebulae: an eye to the future: Programme & abstracts. 2011 ;[citado 2024 ago. 02 ]
Vancouver
Cavichia O, Costa RD'AD da, Molla M, Maciel WJ. Planetary nebulae and the chemical evolution of the galactic bulge: new abundances of older objects. Planetary nebulae: an eye to the future: Programme & abstracts. 2011 ;[citado 2024 ago. 02 ]
Trabalho de evento-resumo
Radial abundance gradients from planetary nebulae and young objects: age effects (2011)
Maciel, Walter Junqueira; Rodrigues, T. S; Costa, Roberto Dell'Aglio Dias da
Fonte: Planetary nebulae: an eye to the future: Programme & abstracts. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ABUNDÂNCIAS (ASTRONOMIA), PLANETAS, GALÁXIA (VIA LÁCTEA)
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ABNT
MACIEL, Walter Junqueira e RODRIGUES, T. S e COSTA, Roberto Dell'Aglio Dias da. Radial abundance gradients from planetary nebulae and young objects: age effects. 2011, Anais.. Paris: International Astronomical Union, 2011. . Acesso em: 02 ago. 2024.
APA
Maciel, W. J., Rodrigues, T. S., & Costa, R. D. 'A. D. da. (2011). Radial abundance gradients from planetary nebulae and young objects: age effects. In Planetary nebulae: an eye to the future: Programme & abstracts. Paris: International Astronomical Union.
NLM
Maciel WJ, Rodrigues TS, Costa RD'AD da. Radial abundance gradients from planetary nebulae and young objects: age effects. Planetary nebulae: an eye to the future: Programme & abstracts. 2011 ;[citado 2024 ago. 02 ]
Vancouver
Maciel WJ, Rodrigues TS, Costa RD'AD da. Radial abundance gradients from planetary nebulae and young objects: age effects. Planetary nebulae: an eye to the future: Programme & abstracts. 2011 ;[citado 2024 ago. 02 ]
Trabalho de evento
Tidal evolution of a close-in planet with a more massive outer companion (2011)
Rodríguez, Adrian; Ferraz-Mello, Sylvio; Michtchenko, Tatiana Alexandrovna; Beaugé, Cristian; Miloni, Octavio
Fonte: The astrophysics of planetary systems: formation, structure and dynamical evolution: Proceedings. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: MECÂNICA CELESTE, PLANETAS
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ABNT
RODRÍGUEZ, Adrian et al. Tidal evolution of a close-in planet with a more massive outer companion. 2011, Anais.. Paris: International Astronomical Union, 2011. Disponível em: https://doi.org/10.1017/S1743921311021004. Acesso em: 02 ago. 2024.
APA
Rodríguez, A., Ferraz-Mello, S., Michtchenko, T. A., Beaugé, C., & Miloni, O. (2011). Tidal evolution of a close-in planet with a more massive outer companion. In The astrophysics of planetary systems: formation, structure and dynamical evolution: Proceedings. Paris: International Astronomical Union. doi:10.1017/S1743921311021004
NLM
Rodríguez A, Ferraz-Mello S, Michtchenko TA, Beaugé C, Miloni O. Tidal evolution of a close-in planet with a more massive outer companion [Internet]. The astrophysics of planetary systems: formation, structure and dynamical evolution: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311021004
Vancouver
Rodríguez A, Ferraz-Mello S, Michtchenko TA, Beaugé C, Miloni O. Tidal evolution of a close-in planet with a more massive outer companion [Internet]. The astrophysics of planetary systems: formation, structure and dynamical evolution: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311021004
Trabalho de evento
Analysing VLBI images of astrophysical jets via cross-entropy global optimisation method (2011)
Caproni, Anderson; Monteiro, Hektor; Abraham, Zulema
Fonte: Jets at all scales: Proceedings. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ANÁLISE DE DADOS, INTERFEROMETRIA, GALÁXIAS ATIVAS, GALÁXIAS, JATOS (ASTRONOMIA)
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ABNT
CAPRONI, Anderson e MONTEIRO, Hektor e ABRAHAM, Zulema. Analysing VLBI images of astrophysical jets via cross-entropy global optimisation method. 2011, Anais.. Paris: International Astronomical Union, 2011. Disponível em: https://doi.org/10.1017/S1743921310015917. Acesso em: 02 ago. 2024.
APA
Caproni, A., Monteiro, H., & Abraham, Z. (2011). Analysing VLBI images of astrophysical jets via cross-entropy global optimisation method. In Jets at all scales: Proceedings. Paris: International Astronomical Union. doi:10.1017/S1743921310015917
NLM
Caproni A, Monteiro H, Abraham Z. Analysing VLBI images of astrophysical jets via cross-entropy global optimisation method [Internet]. Jets at all scales: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921310015917
Vancouver
Caproni A, Monteiro H, Abraham Z. Analysing VLBI images of astrophysical jets via cross-entropy global optimisation method [Internet]. Jets at all scales: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921310015917
Trabalho de evento
Properties of the circumstellar dust in galactic FS CMa objects (2011)
Miroshnichenko, Anatoly S.; Gray, Richard O; Bjorkman, Karen S.; Rudy, Richard J; Lynch, David K; Carciofi, Alex Cavaliéri
Fonte: Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESTRELAS, INFRAVERMELHO, POEIRA INTERESTELAR
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
MIROSHNICHENKO, Anatoly S. et al. Properties of the circumstellar dust in galactic FS CMa objects. 2011, Anais.. Paris: International Astronomical Union, 2011. Disponível em: https://doi.org/10.1017/S1743921311010970. Acesso em: 02 ago. 2024.
APA
Miroshnichenko, A. S., Gray, R. O., Bjorkman, K. S., Rudy, R. J., Lynch, D. K., & Carciofi, A. C. (2011). Properties of the circumstellar dust in galactic FS CMa objects. In Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Paris: International Astronomical Union. doi:10.1017/S1743921311010970
NLM
Miroshnichenko AS, Gray RO, Bjorkman KS, Rudy RJ, Lynch DK, Carciofi AC. Properties of the circumstellar dust in galactic FS CMa objects [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311010970
Vancouver
Miroshnichenko AS, Gray RO, Bjorkman KS, Rudy RJ, Lynch DK, Carciofi AC. Properties of the circumstellar dust in galactic FS CMa objects [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311010970
Trabalho de evento
The circumstellar discs of Be stars (2011)
Carciofi, Alex Cavaliéri
Fonte: Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESTRELAS, ASTROFÍSICA ESTELAR
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
CARCIOFI, Alex Cavaliéri. The circumstellar discs of Be stars. 2011, Anais.. Paris: International Astronomical Union, 2011. Disponível em: https://doi.org/10.1017/S1743921311010738. Acesso em: 02 ago. 2024.
APA
Carciofi, A. C. (2011). The circumstellar discs of Be stars. In Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Paris: International Astronomical Union. doi:10.1017/S1743921311010738
NLM
Carciofi AC. The circumstellar discs of Be stars [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311010738
Vancouver
Carciofi AC. The circumstellar discs of Be stars [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311010738
Trabalho de evento
Particle acceleration in fast magnetic reconnection (2011)
Lazarian, A; Kowal, G; Gouveia dal Pino, Elisabete Maria de; Vishniac, E
Fonte: Advances in plasma astrophysics: Proceedings. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: RAIOS CÓSMICOS, CAMPO MAGNÉTICO, ACELERAÇÃO DE PARTICULAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
LAZARIAN, A et al. Particle acceleration in fast magnetic reconnection. 2011, Anais.. Paris: International Astronomical Union, 2011. Disponível em: https://doi.org/10.1017/S1743921311006582. Acesso em: 02 ago. 2024.
APA
Lazarian, A., Kowal, G., Gouveia dal Pino, E. M. de, & Vishniac, E. (2011). Particle acceleration in fast magnetic reconnection. In Advances in plasma astrophysics: Proceedings. Paris: International Astronomical Union. doi:10.1017/S1743921311006582
NLM
Lazarian A, Kowal G, Gouveia dal Pino EM de, Vishniac E. Particle acceleration in fast magnetic reconnection [Internet]. Advances in plasma astrophysics: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311006582
Vancouver
Lazarian A, Kowal G, Gouveia dal Pino EM de, Vishniac E. Particle acceleration in fast magnetic reconnection [Internet]. Advances in plasma astrophysics: Proceedings. 2011 ;[citado 2024 ago. 02 ] Available from: https://doi.org/10.1017/S1743921311006582

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