Filtros : "AMORIM, TAJAN HENRIQUE DE" "Produção científica" Limpar

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  • Source: Galaxies. Unidades: IAG, ECA

    Subjects: ESTRELAS BINÁRIAS, ESTRELAS VARIÁVEIS

    Acesso à fonteDOIHow to cite
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    • ABNT

      CARCIOFI, Alex Cavaliéri et al. Mass Loss in Be Stars: News from Two Fronts. Galaxies, v. 13, p. 77, 2025Tradução . . Disponível em: https://doi.org/10.3390/galaxies13040077. Acesso em: 10 out. 2025.
    • APA

      Carciofi, A. C., Bolzan, G. P. P., Querido, P. R., Rubio, A. C., Labadie-Bartz, J., Amorin, T. H. de, et al. (2025). Mass Loss in Be Stars: News from Two Fronts. Galaxies, 13, 77. doi:10.3390/galaxies13040077
    • NLM

      Carciofi AC, Bolzan GPP, Querido PR, Rubio AC, Labadie-Bartz J, Amorin TH de, Silva ACF, Schiavolim VL, Carciofi AC. Mass Loss in Be Stars: News from Two Fronts [Internet]. Galaxies. 2025 ;13 77.[citado 2025 out. 10 ] Available from: https://doi.org/10.3390/galaxies13040077
    • Vancouver

      Carciofi AC, Bolzan GPP, Querido PR, Rubio AC, Labadie-Bartz J, Amorin TH de, Silva ACF, Schiavolim VL, Carciofi AC. Mass Loss in Be Stars: News from Two Fronts [Internet]. Galaxies. 2025 ;13 77.[citado 2025 out. 10 ] Available from: https://doi.org/10.3390/galaxies13040077
  • Source: ASTRONOMY & ASTROPHYSICS. Unidade: IAG

    Subjects: ESTRELAS BINÁRIAS, ASTROFÍSICA ESTELAR

    Acesso à fonteDOIHow to cite
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    • ABNT

      RUBIO, Amanda Caveagna et al. High-spatial-resolution simulations of Be star disks in binary systems: I. Structure and kinematics of coplanar disks. ASTRONOMY & ASTROPHYSICS, v. 698, p. A309, 2025Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/202452724. Acesso em: 10 out. 2025.
    • APA

      Rubio, A. C., Carciofi, A. C., Carciofi, A. C., Bjorkman, J. E., Amorim, T. H. de, Okazaki, A. T., et al. (2025). High-spatial-resolution simulations of Be star disks in binary systems: I. Structure and kinematics of coplanar disks. ASTRONOMY & ASTROPHYSICS, 698, A309. doi:10.1051/0004-6361/202452724
    • NLM

      Rubio AC, Carciofi AC, Carciofi AC, Bjorkman JE, Amorim TH de, Okazaki AT, Suffak MW, Jones CE, Candido PP. High-spatial-resolution simulations of Be star disks in binary systems: I. Structure and kinematics of coplanar disks [Internet]. ASTRONOMY & ASTROPHYSICS. 2025 ; 698 A309.[citado 2025 out. 10 ] Available from: https://doi.org/10.1051/0004-6361/202452724
    • Vancouver

      Rubio AC, Carciofi AC, Carciofi AC, Bjorkman JE, Amorim TH de, Okazaki AT, Suffak MW, Jones CE, Candido PP. High-spatial-resolution simulations of Be star disks in binary systems: I. Structure and kinematics of coplanar disks [Internet]. ASTRONOMY & ASTROPHYSICS. 2025 ; 698 A309.[citado 2025 out. 10 ] Available from: https://doi.org/10.1051/0004-6361/202452724
  • Source: ASTRONOMY & ASTROPHYSICS. Unidade: IAG

    Subjects: ESTRELAS BINÁRIAS, ASTROFÍSICA ESTELAR

    Acesso à fonteDOIHow to cite
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    • ABNT

      GAO, Qing et al. A Be star that turned bright and blue during a major outburst. ASTRONOMY & ASTROPHYSICS, v. 694, p. A131, 2025Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/202452792. Acesso em: 10 out. 2025.
    • APA

      Gao, Q., Carciofi, A. C., Wang, W., Baade, D., Amorim, T. H. de, & Carciofi, A. C. (2025). A Be star that turned bright and blue during a major outburst. ASTRONOMY & ASTROPHYSICS, 694, A131. doi:10.1051/0004-6361/202452792
    • NLM

      Gao Q, Carciofi AC, Wang W, Baade D, Amorim TH de, Carciofi AC. A Be star that turned bright and blue during a major outburst [Internet]. ASTRONOMY & ASTROPHYSICS. 2025 ; 694 A131.[citado 2025 out. 10 ] Available from: https://doi.org/10.1051/0004-6361/202452792
    • Vancouver

      Gao Q, Carciofi AC, Wang W, Baade D, Amorim TH de, Carciofi AC. A Be star that turned bright and blue during a major outburst [Internet]. ASTRONOMY & ASTROPHYSICS. 2025 ; 694 A131.[citado 2025 out. 10 ] Available from: https://doi.org/10.1051/0004-6361/202452792
  • Source: Monthly notices of the royal astronomical society. Unidade: IAG

    Subjects: POLARIZAÇÃO (ASTRONOMIA), TRANSFERÊNCIA RADIATIVA

    Acesso à fonteDOIHow to cite
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    • ABNT

      SERIACOPI, D B et al. Multitechnique study of the B[e] supergiant RMC-82. Monthly notices of the royal astronomical society, v. 528, p. 122-140, 2024Tradução . . Disponível em: https://doi.org/10.1093/mnras/stad3948. Acesso em: 10 out. 2025.
    • APA

      SERIACOPI, D. B., Carciofi, A. C., DE AMORIM, T. H., Magalhães, A. M., VIEIRA, R. G., DE SOUZA, A. D. O. M. I. C. I. A. N. O., et al. (2024). Multitechnique study of the B[e] supergiant RMC-82. Monthly notices of the royal astronomical society, 528, 122-140. doi:10.1093/mnras/stad3948
    • NLM

      SERIACOPI DB, Carciofi AC, DE AMORIM TH, Magalhães AM, VIEIRA RG, DE SOUZA ADOMICIANO, RUBIO A, RUBINHO MS, Bednarski D, Mota BC, Faes D, Silva ACF. Multitechnique study of the B[e] supergiant RMC-82 [Internet]. Monthly notices of the royal astronomical society. 2024 ;528 122-140.[citado 2025 out. 10 ] Available from: https://doi.org/10.1093/mnras/stad3948
    • Vancouver

      SERIACOPI DB, Carciofi AC, DE AMORIM TH, Magalhães AM, VIEIRA RG, DE SOUZA ADOMICIANO, RUBIO A, RUBINHO MS, Bednarski D, Mota BC, Faes D, Silva ACF. Multitechnique study of the B[e] supergiant RMC-82 [Internet]. Monthly notices of the royal astronomical society. 2024 ;528 122-140.[citado 2025 out. 10 ] Available from: https://doi.org/10.1093/mnras/stad3948
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ESTRELAS BINÁRIAS, TRANSFERÊNCIA RADIATIVA

    Acesso à fonteDOIHow to cite
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    • ABNT

      SUFFAK, M W et al. Non-LTE Monte Carlo radiative transfer.: III. the thermal properties of tilted and warped be star discs. Monthly Notices of the Royal Astronomical Society, 2023Tradução . . Disponível em: https://doi.org/10.1093/mnras/stad2781. Acesso em: 10 out. 2025.
    • APA

      Suffak, M. W., Jones, C. E., Carciofi, A. C., & Amorim, T. H. (2023). Non-LTE Monte Carlo radiative transfer.: III. the thermal properties of tilted and warped be star discs. Monthly Notices of the Royal Astronomical Society. doi:10.1093/mnras/stad2781
    • NLM

      Suffak MW, Jones CE, Carciofi AC, Amorim TH. Non-LTE Monte Carlo radiative transfer.: III. the thermal properties of tilted and warped be star discs [Internet]. Monthly Notices of the Royal Astronomical Society. 2023 ;[citado 2025 out. 10 ] Available from: https://doi.org/10.1093/mnras/stad2781
    • Vancouver

      Suffak MW, Jones CE, Carciofi AC, Amorim TH. Non-LTE Monte Carlo radiative transfer.: III. the thermal properties of tilted and warped be star discs [Internet]. Monthly Notices of the Royal Astronomical Society. 2023 ;[citado 2025 out. 10 ] Available from: https://doi.org/10.1093/mnras/stad2781
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Assunto: ESTRELAS BINÁRIAS

    Acesso à fonteDOIHow to cite
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    • ABNT

      RUBIO, A. C et al. Bayesian sampling with BeAtlas, a grid of synthetic Be star spectra: I. Recovering the fundamental parameters of 𝛼 Eri and 𝛽 CMi. Monthly Notices of the Royal Astronomical Society, 2023Tradução . . Disponível em: https://doi.org/10.1093/mnras/stad2652. Acesso em: 10 out. 2025.
    • APA

      Rubio, A. C., Carciofi, A. C., Ticiani, P., Mota, B. C., Amorim, T. H., & Silva, A. C. F. (2023). Bayesian sampling with BeAtlas, a grid of synthetic Be star spectra: I. Recovering the fundamental parameters of 𝛼 Eri and 𝛽 CMi. Monthly Notices of the Royal Astronomical Society. doi:10.1093/mnras/stad2652
    • NLM

      Rubio AC, Carciofi AC, Ticiani P, Mota BC, Amorim TH, Silva ACF. Bayesian sampling with BeAtlas, a grid of synthetic Be star spectra: I. Recovering the fundamental parameters of 𝛼 Eri and 𝛽 CMi [Internet]. Monthly Notices of the Royal Astronomical Society. 2023 ;[citado 2025 out. 10 ] Available from: https://doi.org/10.1093/mnras/stad2652
    • Vancouver

      Rubio AC, Carciofi AC, Ticiani P, Mota BC, Amorim TH, Silva ACF. Bayesian sampling with BeAtlas, a grid of synthetic Be star spectra: I. Recovering the fundamental parameters of 𝛼 Eri and 𝛽 CMi [Internet]. Monthly Notices of the Royal Astronomical Society. 2023 ;[citado 2025 out. 10 ] Available from: https://doi.org/10.1093/mnras/stad2652

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