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Filtros : "Universidad Nacional de La Plata (UNLP)" "The Astrophysical Journal" Removido: "FCF001" Limpar

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  • Artigo de periodico

    The quasi-roche lobe overflow state in the evolution of close binary systems containing a radio pulsar (2015)

    Benvenuto, O. G; De Vito, M. A; Horvath, Jorge Ernesto

    Source: The Astrophysical Journal. Unidade: IAG

    Subjects: ESTRELAS, ESTRELAS BINÁRIAS, PULSARES, EVOLUÇÃO ESTELAR

    Acesso à fonteDOIHow to cite
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    • ABNT

      BENVENUTO, O. G e DE VITO, M. A e HORVATH, Jorge Ernesto. The quasi-roche lobe overflow state in the evolution of close binary systems containing a radio pulsar. The Astrophysical Journal, v. 798, p. 44/1-44/8, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/798/1/44. Acesso em: 18 out. 2024.

    • APA

      Benvenuto, O. G., De Vito, M. A., & Horvath, J. E. (2015). The quasi-roche lobe overflow state in the evolution of close binary systems containing a radio pulsar. The Astrophysical Journal, 798, 44/1-44/8. doi:10.1088/0004-637X/798/1/44

    • NLM

      Benvenuto OG, De Vito MA, Horvath JE. The quasi-roche lobe overflow state in the evolution of close binary systems containing a radio pulsar [Internet]. The Astrophysical Journal. 2015 ; 798 44/1-44/8.[citado 2024 out. 18 ] Available from: https://doi.org/10.1088/0004-637X/798/1/44

    • Vancouver

      Benvenuto OG, De Vito MA, Horvath JE. The quasi-roche lobe overflow state in the evolution of close binary systems containing a radio pulsar [Internet]. The Astrophysical Journal. 2015 ; 798 44/1-44/8.[citado 2024 out. 18 ] Available from: https://doi.org/10.1088/0004-637X/798/1/44

  • Artigo de periodico

    Bona fide, strong-variable galactic luminous blue variable stars are fast rotators: detection of a high rotational velocity in HR Carinae (2009)

    Groh, J.H; Barbá, R; Damineli Neto, Augusto; Hillier, D.J; Fernández-Lajús; Gamen, R. C; Moisés, A. P; Solivella, G; Teodoro, M

    Source: The Astrophysical Journal. Unidade: IAG

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

    How to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas

    • ABNT

      GROH, J.H et al. Bona fide, strong-variable galactic luminous blue variable stars are fast rotators: detection of a high rotational velocity in HR Carinae. The Astrophysical Journal, v. 705, p. L25-L30, 2009Tradução . . Acesso em: 18 out. 2024.

    • APA

      Groh, J. H., Barbá, R., Damineli Neto, A., Hillier, D. J., Fernández-Lajús,, Gamen, R. C., et al. (2009). Bona fide, strong-variable galactic luminous blue variable stars are fast rotators: detection of a high rotational velocity in HR Carinae. The Astrophysical Journal, 705, L25-L30.

    • NLM

      Groh JH, Barbá R, Damineli Neto A, Hillier DJ, Fernández-Lajús, Gamen RC, Moisés AP, Solivella G, Teodoro M. Bona fide, strong-variable galactic luminous blue variable stars are fast rotators: detection of a high rotational velocity in HR Carinae. The Astrophysical Journal. 2009 ; 705 L25-L30.[citado 2024 out. 18 ]

    • Vancouver

      Groh JH, Barbá R, Damineli Neto A, Hillier DJ, Fernández-Lajús, Gamen RC, Moisés AP, Solivella G, Teodoro M. Bona fide, strong-variable galactic luminous blue variable stars are fast rotators: detection of a high rotational velocity in HR Carinae. The Astrophysical Journal. 2009 ; 705 L25-L30.[citado 2024 out. 18 ]
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