Filtros : "IAG" "IAU Symposium" Removidos: "Boletim da Sociedade Astronomica Brasileira" "GONCALVES, FABIO LUIZ TEIXEIRA" Limpar

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  • Source: Proceedings of the International Astronomical Union: From Interacting Binaries to Exoplanets: Essential Modeling Tools. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: ESTRELAS BINÁRIAS, PERDA DE MASSA, VENTO, ESTRELAS

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      MENNICKENT, Ronald E et al. Optical spectroscopy of V393 Scorpii during its long cycle. 2012, Anais.. Paris: International Astronomical Union, 2012. Disponível em: https://doi.org/10.1017/S1743921311027694. Acesso em: 23 abr. 2024.
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      Mennickent, R. E., Kolaczkowski, Z., Djurasevic, G., Diaz, M. P., & Niemczura, E. (2012). Optical spectroscopy of V393 Scorpii during its long cycle. In Proceedings of the International Astronomical Union: From Interacting Binaries to Exoplanets: Essential Modeling Tools. Paris: International Astronomical Union. doi:10.1017/S1743921311027694
    • NLM

      Mennickent RE, Kolaczkowski Z, Djurasevic G, Diaz MP, Niemczura E. Optical spectroscopy of V393 Scorpii during its long cycle [Internet]. Proceedings of the International Astronomical Union: From Interacting Binaries to Exoplanets: Essential Modeling Tools. 2012 ;[citado 2024 abr. 23 ] Available from: https://doi.org/10.1017/S1743921311027694
    • Vancouver

      Mennickent RE, Kolaczkowski Z, Djurasevic G, Diaz MP, Niemczura E. Optical spectroscopy of V393 Scorpii during its long cycle [Internet]. Proceedings of the International Astronomical Union: From Interacting Binaries to Exoplanets: Essential Modeling Tools. 2012 ;[citado 2024 abr. 23 ] Available from: https://doi.org/10.1017/S1743921311027694
  • Source: Proceedings of the International Astronomical Union: Planetary nebulae: an eye to the future. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: NEBULOSAS, GALÁXIAS, ABUNDÂNCIAS (ASTRONOMIA), FORMAÇÃO E EVOLUÇÃO DA GALÁXIA

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      CAVICHIA, O et al. Planetary nebulae and the chemical evolution of the galactic bulge: new abundances of older objects. 2012, Anais.. Paris: International Astronomical Union, 2012. Disponível em: https://doi.org/10.1017/S1743921312011258. Acesso em: 23 abr. 2024.
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      Cavichia, O., Costa, R. D. 'A. D. da, Mollá, M., & Maciel, W. J. (2012). Planetary nebulae and the chemical evolution of the galactic bulge: new abundances of older objects. In Proceedings of the International Astronomical Union: Planetary nebulae: an eye to the future. Paris: International Astronomical Union. doi:10.1017/S1743921312011258
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      Cavichia O, Costa RD'AD da, Mollá M, Maciel WJ. Planetary nebulae and the chemical evolution of the galactic bulge: new abundances of older objects [Internet]. Proceedings of the International Astronomical Union: Planetary nebulae: an eye to the future. 2012 ;[citado 2024 abr. 23 ] Available from: https://doi.org/10.1017/S1743921312011258
    • Vancouver

      Cavichia O, Costa RD'AD da, Mollá M, Maciel WJ. Planetary nebulae and the chemical evolution of the galactic bulge: new abundances of older objects [Internet]. Proceedings of the International Astronomical Union: Planetary nebulae: an eye to the future. 2012 ;[citado 2024 abr. 23 ] Available from: https://doi.org/10.1017/S1743921312011258
  • Source: Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: ABUNDÂNCIAS (ASTRONOMIA), PLANETAS, GALÁXIA (VIA LÁCTEA)

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      MACIEL, Walter Junqueira e RODRIGUES, Thaise e COSTA, Roberto Dell'Aglio Dias da. Radial abundance gradients from planetary nebulae and young objects: age effects. 2012, Anais.. Paris: International Astronomical Union, 2012. Disponível em: https://doi.org/10.1017/S174392131201174X. Acesso em: 23 abr. 2024.
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      Maciel, W. J., Rodrigues, T., & Costa, R. D. 'A. D. da. (2012). Radial abundance gradients from planetary nebulae and young objects: age effects. In Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Paris: International Astronomical Union. doi:10.1017/S174392131201174X
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      Maciel WJ, Rodrigues T, Costa RD'AD da. Radial abundance gradients from planetary nebulae and young objects: age effects [Internet]. Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. 2012 ;[citado 2024 abr. 23 ] Available from: https://doi.org/10.1017/S174392131201174X
    • Vancouver

      Maciel WJ, Rodrigues T, Costa RD'AD da. Radial abundance gradients from planetary nebulae and young objects: age effects [Internet]. Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. 2012 ;[citado 2024 abr. 23 ] Available from: https://doi.org/10.1017/S174392131201174X
  • Source: Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: NEBULOSAS, PLANETAS, ESTRELAS

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      RODRIGUES, Thaise S e MACIEL, Walter Junqueira. Kinematic age determinations of planetary nebula central stars. 2012, Anais.. Paris: International Astronomical Union, 2012. Disponível em: https://doi.org/10.1017/S1743921312012057. Acesso em: 23 abr. 2024.
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      Rodrigues, T. S., & Maciel, W. J. (2012). Kinematic age determinations of planetary nebula central stars. In Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Paris: International Astronomical Union. doi:10.1017/S1743921312012057
    • NLM

      Rodrigues TS, Maciel WJ. Kinematic age determinations of planetary nebula central stars [Internet]. Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. 2012 ;[citado 2024 abr. 23 ] Available from: https://doi.org/10.1017/S1743921312012057
    • Vancouver

      Rodrigues TS, Maciel WJ. Kinematic age determinations of planetary nebula central stars [Internet]. Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. 2012 ;[citado 2024 abr. 23 ] Available from: https://doi.org/10.1017/S1743921312012057
  • Source: Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: ESTRELAS, ATMOSFERAS ESTELARES, PERDA DE MASSA, VENTO

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      KELLER, Graziela R et al. Grids of synthetic spectra for H-poor central stars of planetary nebulae (CSPNe). 2012, Anais.. Paris: International Astronomical Union, 2012. Disponível em: https://doi.org/10.1017/S1743921312011647. Acesso em: 23 abr. 2024.
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      Keller, G. R., Bianchi, L., Herald, J. E., & Maciel, W. J. (2012). Grids of synthetic spectra for H-poor central stars of planetary nebulae (CSPNe). In Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Paris: International Astronomical Union. doi:10.1017/S1743921312011647
    • NLM

      Keller GR, Bianchi L, Herald JE, Maciel WJ. Grids of synthetic spectra for H-poor central stars of planetary nebulae (CSPNe) [Internet]. Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. 2012 ;[citado 2024 abr. 23 ] Available from: https://doi.org/10.1017/S1743921312011647
    • Vancouver

      Keller GR, Bianchi L, Herald JE, Maciel WJ. Grids of synthetic spectra for H-poor central stars of planetary nebulae (CSPNe) [Internet]. Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. 2012 ;[citado 2024 abr. 23 ] Available from: https://doi.org/10.1017/S1743921312011647
  • Source: Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: ESPECTROSCOPIA, NEBULOSAS, ASTROQUÍMICA

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      COSTA, Roberto Dell'Aglio Dias da e FAES, Daniel M e MORISSET, Christophe. Physical parameters and chemical abundances in bipolar PNe. 2012, Anais.. Paris: International Astronomical Union, 2012. Disponível em: https://doi.org/10.1017/S1743921312011301. Acesso em: 23 abr. 2024.
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      Costa, R. D. 'A. D. da, Faes, D. M., & Morisset, C. (2012). Physical parameters and chemical abundances in bipolar PNe. In Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Paris: International Astronomical Union. doi:10.1017/S1743921312011301
    • NLM

      Costa RD'AD da, Faes DM, Morisset C. Physical parameters and chemical abundances in bipolar PNe [Internet]. Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. 2012 ;[citado 2024 abr. 23 ] Available from: https://doi.org/10.1017/S1743921312011301
    • Vancouver

      Costa RD'AD da, Faes DM, Morisset C. Physical parameters and chemical abundances in bipolar PNe [Internet]. Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. 2012 ;[citado 2024 abr. 23 ] Available from: https://doi.org/10.1017/S1743921312011301
  • Source: Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: ESTRELAS, ASTROFÍSICA ESTELAR

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      JANOT PACHECO, Eduardo et al. Non-radial pulsations in the CoRoT Be Star 102761769. 2011, Anais.. Paris: International Astronomical Union, 2011. . Acesso em: 23 abr. 2024.
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      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 abr. 23 ]
    • 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 abr. 23 ]
  • Source: Planetary nebulae: an eye to the future: Programme & abstracts. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: ESTRELAS, NEBULOSAS, PLANETAS, MEIO INTERESTELAR

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      RODRIGUES, T. S e MACIEL, Walter Junqueira. Kenematic age determinations of planetary nebula central stars. 2011, Anais.. Paris: International Astronomical Union, 2011. . Acesso em: 23 abr. 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 abr. 23 ]
    • 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 abr. 23 ]
  • Source: Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: ESTRELAS, ASTROFÍSICA ESTELAR

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      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: 23 abr. 2024.
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      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
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      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 abr. 23 ] 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 abr. 23 ] Available from: https://doi.org/10.1017/S1743921311011483
  • Source: Active OB stars : structure, evolution, mass loss, and critical limits: proceedings. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: TRANSFERÊNCIA RADIATIVA, ESTRELAS, EVOLUÇÃO ESTELAR

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      HAUBOIS, Xavier et al. The dynamical evolution of Be star disks. 2011, Anais.. Paris: International Astronomical Union, 2011. . Acesso em: 23 abr. 2024.
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      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 abr. 23 ]
    • 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 abr. 23 ]
  • Source: The spectral energy distribution of galaxies (SED 2011): Abstracts. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: FORMAÇÃO DE ESTRELAS, GALÁXIA (VIA LÁCTEA)

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      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: 23 abr. 2024.
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      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.
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      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 abr. 23 ]
    • 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 abr. 23 ]
  • Source: Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: ESTRELAS, ESTRELAS VARIÁVEIS, ESTRELAS BINÁRIAS

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      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: 23 abr. 2024.
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      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
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      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 abr. 23 ] 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 abr. 23 ] Available from: https://doi.org/10.1017/S1743921311011513
  • Source: Advances in plasma astrophysics: Proceedings. Conference titles: IAU Symposium. Unidades: IAG, EACH

    Subjects: CAMPO MAGNÉTICO, MEIO INTERGALÁTICO, PLASMA, MAGNETOHIDRODINÂMICA

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      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: 23 abr. 2024.
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      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 abr. 23 ] 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 abr. 23 ] Available from: https://doi.org/10.1017/S1743921311007563
  • Source: Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: ESTRELAS, POLARIZAÇÃO (ASTRONOMIA)

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      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: 23 abr. 2024.
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      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
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      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 abr. 23 ] 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 abr. 23 ] Available from: https://doi.org/10.1017/S1743921311010854
  • Source: Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: ESTRELAS, VENTO, POEIRA INTERESTELAR

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      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: 23 abr. 2024.
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      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
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      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 abr. 23 ] 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 abr. 23 ] Available from: https://doi.org/10.1017/S1743921311010830
  • Source: Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: ESTRELAS, ESPECTROS, ASTROFÍSICA ESTELAR

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      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: 23 abr. 2024.
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      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 abr. 23 ] 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 abr. 23 ] Available from: https://doi.org/10.1017/S1743921311011008
  • Source: Jets at all scales: Proceedings. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: ESTRELAS BINÁRIAS, ESPECTROSCOPIA, ESTRELAS NOVAS

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      TOVMASSIAN, G et al. Do cataclysmic variables produce jets? 2011, Anais.. Paris: International Astronomical Union, 2011. . Acesso em: 23 abr. 2024.
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      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 abr. 23 ]
    • Vancouver

      Tovmassian G, Gänsicke B, Zharikov S, Ramírez A, Diaz MP. Do cataclysmic variables produce jets? Jets at all scales: Proceedings. 2011 ;[citado 2024 abr. 23 ]
  • Source: Planetary nebulae: an eye to the future: Programme & abstracts. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: PLANETAS, NEBULOSAS

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      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: 23 abr. 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 abr. 23 ]
    • 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 abr. 23 ]
  • Source: Jets at all scales: Proceedings. Conference titles: IAU Symposium. Unidades: IAG, EACH

    Subjects: GALÁXIAS, JATOS (ASTRONOMIA), DISCOS DE ACRESÇÂO

    Acesso à fonteDOIHow to cite
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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: 23 abr. 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 abr. 23 ] 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 abr. 23 ] Available from: https://doi.org/10.1017/S1743921310015954
  • Source: Planetary nebulae: an eye to the future: Programme & abstracts. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: FORMAÇÃO E EVOLUÇÃO DA GALÁXIA, NEBULOSAS

    How to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • 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: 23 abr. 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 abr. 23 ]
    • 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 abr. 23 ]

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