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  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: MÉTODOS NUMÉRICOS, TRANSFERÊNCIA RADIATIVA, ESTRELAS, CINEMÁTICA, DINÂMICA

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    • ABNT

      ESCOLANO, C et al. 2.5D global-disk oscillation models of the Be shell star 'dzeta' Tauri: I. Spectroscopic and polarimetric analysis. Astronomy & Astrophysics, v. 576, p. A112/1-A112/15, 2015Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201425446. Acesso em: 05 nov. 2024.
    • APA

      Escolano, C., Carciofi, A. C., Okazaki, A. T., Rivinius, T., Baade, D., & Štefl, S. (2015). 2.5D global-disk oscillation models of the Be shell star 'dzeta' Tauri: I. Spectroscopic and polarimetric analysis. Astronomy & Astrophysics, 576, A112/1-A112/15. doi:10.1051/0004-6361/201425446
    • NLM

      Escolano C, Carciofi AC, Okazaki AT, Rivinius T, Baade D, Štefl S. 2.5D global-disk oscillation models of the Be shell star 'dzeta' Tauri: I. Spectroscopic and polarimetric analysis [Internet]. Astronomy & Astrophysics. 2015 ; 576 A112/1-A112/15.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1051/0004-6361/201425446
    • Vancouver

      Escolano C, Carciofi AC, Okazaki AT, Rivinius T, Baade D, Štefl S. 2.5D global-disk oscillation models of the Be shell star 'dzeta' Tauri: I. Spectroscopic and polarimetric analysis [Internet]. Astronomy & Astrophysics. 2015 ; 576 A112/1-A112/15.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1051/0004-6361/201425446
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS, MÉTODOS NUMÉRICOS, INTERFEROMETRIA

    Acesso à fonteDOIHow to cite
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    • ABNT

      DOMICIANO DE SOUZA, A et al. The environment of the fast rotating star Achernar: III. Photospheric parameters revealed by the VLTI. Astronomy & Astrophysics, v. 569, p. A10/1-A10/15, 2014Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201424144. Acesso em: 05 nov. 2024.
    • APA

      Domiciano de Souza, A., Kervella, P., Moser Faes, D., Dalla Vedova, G., Mérand, A., Le Bouquin J.-B,, et al. (2014). The environment of the fast rotating star Achernar: III. Photospheric parameters revealed by the VLTI. Astronomy & Astrophysics, 569, A10/1-A10/15. doi:10.1051/0004-6361/201424144
    • NLM

      Domiciano de Souza A, Kervella P, Moser Faes D, Dalla Vedova G, Mérand A, Le Bouquin J.-B, Espinosa Lara F, Rieutord M, Bendjoya P, Carciofi AC, Hadjara M, Millour F, Vakili F. The environment of the fast rotating star Achernar: III. Photospheric parameters revealed by the VLTI [Internet]. Astronomy & Astrophysics. 2014 ; 569 A10/1-A10/15.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1051/0004-6361/201424144
    • Vancouver

      Domiciano de Souza A, Kervella P, Moser Faes D, Dalla Vedova G, Mérand A, Le Bouquin J.-B, Espinosa Lara F, Rieutord M, Bendjoya P, Carciofi AC, Hadjara M, Millour F, Vakili F. The environment of the fast rotating star Achernar: III. Photospheric parameters revealed by the VLTI [Internet]. Astronomy & Astrophysics. 2014 ; 569 A10/1-A10/15.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1051/0004-6361/201424144
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ESTRELAS, MÉTODOS NUMÉRICOS, PERDA DE MASSA, VENTO

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    • ABNT

      STEFFEN, W et al. The three-dimensional structure of the Eta Carinae Homunculus. Monthly Notices of the Royal Astronomical Society, v. 442, p. 3316-3328, 2014Tradução . . Disponível em: https://doi.org/10.1093/mnras/stu1088. Acesso em: 05 nov. 2024.
    • APA

      Steffen, W., Teodoro, M., Madura, T. I., Groh, J. H., Gull, T. R., Mehner, A., et al. (2014). The three-dimensional structure of the Eta Carinae Homunculus. Monthly Notices of the Royal Astronomical Society, 442, 3316-3328. doi:10.1093/mnras/stu1088
    • NLM

      Steffen W, Teodoro M, Madura TI, Groh JH, Gull TR, Mehner A, Corcoran MF, Damineli Neto A, Hamaguchi K. The three-dimensional structure of the Eta Carinae Homunculus [Internet]. Monthly Notices of the Royal Astronomical Society. 2014 ; 442 3316-3328.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1093/mnras/stu1088
    • Vancouver

      Steffen W, Teodoro M, Madura TI, Groh JH, Gull TR, Mehner A, Corcoran MF, Damineli Neto A, Hamaguchi K. The three-dimensional structure of the Eta Carinae Homunculus [Internet]. Monthly Notices of the Royal Astronomical Society. 2014 ; 442 3316-3328.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1093/mnras/stu1088
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS, MÉTODOS NUMÉRICOS, INTERFEROMETRIA

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    • ABNT

      DOMICIANO DE SOUZA, A et al. Beyond the diffraction limit of optical/IR interferometers: I. Angular diameter and rotation parameters of Achernar from differential phases. Astronomy & Astrophysics, v. 545, p. A130/1-A130/10, 2012Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201218782. Acesso em: 05 nov. 2024.
    • APA

      Domiciano de Souza, A., Hadjara, M., Vakili, F., Bendjoya, P., Millour, F., Abe, L., et al. (2012). Beyond the diffraction limit of optical/IR interferometers: I. Angular diameter and rotation parameters of Achernar from differential phases. Astronomy & Astrophysics, 545, A130/1-A130/10. doi:10.1051/0004-6361/201218782
    • NLM

      Domiciano de Souza A, Hadjara M, Vakili F, Bendjoya P, Millour F, Abe L, Carciofi AC, Faes DM, Kervella P, Lagarde S, Marconi A, Monin J-L, Niccolini G, Petrov RG, Weigelt G. Beyond the diffraction limit of optical/IR interferometers: I. Angular diameter and rotation parameters of Achernar from differential phases [Internet]. Astronomy & Astrophysics. 2012 ; 545 A130/1-A130/10.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1051/0004-6361/201218782
    • Vancouver

      Domiciano de Souza A, Hadjara M, Vakili F, Bendjoya P, Millour F, Abe L, Carciofi AC, Faes DM, Kervella P, Lagarde S, Marconi A, Monin J-L, Niccolini G, Petrov RG, Weigelt G. Beyond the diffraction limit of optical/IR interferometers: I. Angular diameter and rotation parameters of Achernar from differential phases [Internet]. Astronomy & Astrophysics. 2012 ; 545 A130/1-A130/10.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1051/0004-6361/201218782
  • Source: Monthly Notices of the Royal Astronomical Society. Letters. Unidade: IAG

    Subjects: POLARIZAÇÃO (ASTRONOMIA), MÉTODOS NUMÉRICOS, ESTRELAS

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    • ABNT

      WHEELWRIGHT, H. E et al. Probing the properties of Be star discs with spectroastrometry and NLTE radiative transfer modelling: 'beta' CMi. Monthly Notices of the Royal Astronomical Society. Letters, v. 423, p. L11-L15, 2012Tradução . . Disponível em: https://doi.org/10.1111/j.1745-3933.2012.01241.x. Acesso em: 05 nov. 2024.
    • APA

      Wheelwright, H. E., Bjorkman, J. E., Oudmaijer, R. D., Carciofi, A. C., Bjorkman, K. S., & Porter, J. M. (2012). Probing the properties of Be star discs with spectroastrometry and NLTE radiative transfer modelling: 'beta' CMi. Monthly Notices of the Royal Astronomical Society. Letters, 423, L11-L15. doi:10.1111/j.1745-3933.2012.01241.x
    • NLM

      Wheelwright HE, Bjorkman JE, Oudmaijer RD, Carciofi AC, Bjorkman KS, Porter JM. Probing the properties of Be star discs with spectroastrometry and NLTE radiative transfer modelling: 'beta' CMi [Internet]. Monthly Notices of the Royal Astronomical Society. Letters. 2012 ; 423 L11-L15.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1111/j.1745-3933.2012.01241.x
    • Vancouver

      Wheelwright HE, Bjorkman JE, Oudmaijer RD, Carciofi AC, Bjorkman KS, Porter JM. Probing the properties of Be star discs with spectroastrometry and NLTE radiative transfer modelling: 'beta' CMi [Internet]. Monthly Notices of the Royal Astronomical Society. Letters. 2012 ; 423 L11-L15.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1111/j.1745-3933.2012.01241.x
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS, MÉTODOS NUMÉRICOS, INTERFEROMETRIA

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    • ABNT

      DOMICIANO DE SOUZA, A e CARCIOFI, Alex Cavalieri e FAES, D. M. Beyond the diffraction limit of optical/IR interferometers: I. Angular diameter and rotation parameters of Achernar from differential phases. Astronomy & Astrophysics, v. 545, p. A130/1-A130/10, 2012Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201218782. Acesso em: 05 nov. 2024.
    • APA

      Domiciano de Souza, A., Carciofi, A. C., & Faes, D. M. (2012). Beyond the diffraction limit of optical/IR interferometers: I. Angular diameter and rotation parameters of Achernar from differential phases. Astronomy & Astrophysics, 545, A130/1-A130/10. doi:10.1051/0004-6361/201218782
    • NLM

      Domiciano de Souza A, Carciofi AC, Faes DM. Beyond the diffraction limit of optical/IR interferometers: I. Angular diameter and rotation parameters of Achernar from differential phases [Internet]. Astronomy & Astrophysics. 2012 ; 545 A130/1-A130/10.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1051/0004-6361/201218782
    • Vancouver

      Domiciano de Souza A, Carciofi AC, Faes DM. Beyond the diffraction limit of optical/IR interferometers: I. Angular diameter and rotation parameters of Achernar from differential phases [Internet]. Astronomy & Astrophysics. 2012 ; 545 A130/1-A130/10.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1051/0004-6361/201218782
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS, MÉTODOS NUMÉRICOS, INTERFEROMETRIA, ASTROFÍSICA ESTELAR

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    • ABNT

      SOUZA, A Domiciano de et al. Fast ray-tracing algorithm for circumstellar structures (FRACS): II. Disc parameters of the B[e] supergiant CPD-57º 2874 from VLTI/MIDI data. Astronomy & Astrophysics, v. 525, p. A22/1-A22/11, 2011Tradução . . Acesso em: 05 nov. 2024.
    • APA

      Souza, A. D. de, Bendjoya, P., Niccolini, G., Chesneau, O., Fernandes, M. B., Carciofi, A. C., et al. (2011). Fast ray-tracing algorithm for circumstellar structures (FRACS): II. Disc parameters of the B[e] supergiant CPD-57º 2874 from VLTI/MIDI data. Astronomy & Astrophysics, 525, A22/1-A22/11.
    • NLM

      Souza AD de, Bendjoya P, Niccolini G, Chesneau O, Fernandes MB, Carciofi AC, Spang A, Stee P, Driebe T. Fast ray-tracing algorithm for circumstellar structures (FRACS): II. Disc parameters of the B[e] supergiant CPD-57º 2874 from VLTI/MIDI data. Astronomy & Astrophysics. 2011 ; 525 A22/1-A22/11.[citado 2024 nov. 05 ]
    • Vancouver

      Souza AD de, Bendjoya P, Niccolini G, Chesneau O, Fernandes MB, Carciofi AC, Spang A, Stee P, Driebe T. Fast ray-tracing algorithm for circumstellar structures (FRACS): II. Disc parameters of the B[e] supergiant CPD-57º 2874 from VLTI/MIDI data. Astronomy & Astrophysics. 2011 ; 525 A22/1-A22/11.[citado 2024 nov. 05 ]
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: MÉTODOS NUMÉRICOS, MAGNETOHIDRODINÂMICA, ESTRELAS, VENTO

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    • ABNT

      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: 05 nov. 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 nov. 05 ]
    • 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 nov. 05 ]
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: CAMPO MAGNÉTICO, MÉTODOS NUMÉRICOS, MAGNETOHIDRODINÂMICA, PLANETAS, SATÉLITES, ESTRELAS T TAURI, ESTRELAS, VENTO

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      VIDOTTO, A.A et al. Simulations of winds of weak-lined T Tauri stars: the magnetic field geometry and the influence of the wind on giant planet migration. The Astrophysical Journal, v. 703, p. 1734-1742, 2009Tradução . . Acesso em: 05 nov. 2024.
    • APA

      Vidotto, A. A., Opher, M., Pereira, V. J., & Gombosi, T. I. (2009). Simulations of winds of weak-lined T Tauri stars: the magnetic field geometry and the influence of the wind on giant planet migration. The Astrophysical Journal, 703, 1734-1742.
    • NLM

      Vidotto AA, Opher M, Pereira VJ, Gombosi TI. Simulations of winds of weak-lined T Tauri stars: the magnetic field geometry and the influence of the wind on giant planet migration. The Astrophysical Journal. 2009 ;703 1734-1742.[citado 2024 nov. 05 ]
    • Vancouver

      Vidotto AA, Opher M, Pereira VJ, Gombosi TI. Simulations of winds of weak-lined T Tauri stars: the magnetic field geometry and the influence of the wind on giant planet migration. The Astrophysical Journal. 2009 ;703 1734-1742.[citado 2024 nov. 05 ]

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