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Optical spectroscopy of V393 Scorpii during its long cycle (2012)
Mennickent, Ronald E; Kolaczkowski, Zbigniew; Djurasevic, Gojko; Diaz, Marcos Perez; Niemczura, Ewa
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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
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: 15 set. 2024.
APA
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 set. 15 ] 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 set. 15 ] Available from: https://doi.org/10.1017/S1743921311027694
Artigo de periodico
A cyclic bipolar wind in the interacting binary V 393 Scorpii (2012)
Mennickent, R. E; Kolaczkowski, Z; Djurasevic, G; Niemczura, E; Diaz, Marcos Perez; Curé, M; Araya, I; Peters, G. J
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ESTRELAS BINÁRIAS, ESTRELAS, EVOLUÇÃO ESTELAR, PERDA DE MASSA, VENTO
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
MENNICKENT, R. E et al. A cyclic bipolar wind in the interacting binary V 393 Scorpii. Monthly Notices of the Royal Astronomical Society, v. 427, p. 607-624, 2012Tradução . . Disponível em: https://doi.org/10.1111/j.1365-2966.2012.21309.x. Acesso em: 15 set. 2024.
APA
Mennickent, R. E., Kolaczkowski, Z., Djurasevic, G., Niemczura, E., Diaz, M. P., Curé, M., et al. (2012). A cyclic bipolar wind in the interacting binary V 393 Scorpii. Monthly Notices of the Royal Astronomical Society, 427, 607-624. doi:10.1111/j.1365-2966.2012.21309.x
NLM
Mennickent RE, Kolaczkowski Z, Djurasevic G, Niemczura E, Diaz MP, Curé M, Araya I, Peters GJ. A cyclic bipolar wind in the interacting binary V 393 Scorpii [Internet]. Monthly Notices of the Royal Astronomical Society. 2012 ; 427 607-624.[citado 2024 set. 15 ] Available from: https://doi.org/10.1111/j.1365-2966.2012.21309.x
Vancouver
Mennickent RE, Kolaczkowski Z, Djurasevic G, Niemczura E, Diaz MP, Curé M, Araya I, Peters GJ. A cyclic bipolar wind in the interacting binary V 393 Scorpii [Internet]. Monthly Notices of the Royal Astronomical Society. 2012 ; 427 607-624.[citado 2024 set. 15 ] Available from: https://doi.org/10.1111/j.1365-2966.2012.21309.x
Artigo de periodico
A method for the study of accretion disk emission in cataclysmic variables: I. The model (2011)
Puebla, Raúl E; Diaz, Marcos Perez; Hillier, D. John; Hubeny, Ivan
Source: The Astrophysical Journal. Unidade: IAG
Subjects: DISCOS DE ACRESÇÃO, ESTRELAS, PERDA DE MASSA, RADIAÇÃO ULTRAVIOLETA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
PUEBLA, Raúl E et al. A method for the study of accretion disk emission in cataclysmic variables: I. The model. The Astrophysical Journal, v. 736, p. 17/1-17/18, 2011Tradução . . Acesso em: 15 set. 2024.
APA
Puebla, R. E., Diaz, M. P., Hillier, D. J., & Hubeny, I. (2011). A method for the study of accretion disk emission in cataclysmic variables: I. The model. The Astrophysical Journal, 736, 17/1-17/18.
NLM
Puebla RE, Diaz MP, Hillier DJ, Hubeny I. A method for the study of accretion disk emission in cataclysmic variables: I. The model. The Astrophysical Journal. 2011 ; 736 17/1-17/18.[citado 2024 set. 15 ]
Vancouver
Puebla RE, Diaz MP, Hillier DJ, Hubeny I. A method for the study of accretion disk emission in cataclysmic variables: I. The model. The Astrophysical Journal. 2011 ; 736 17/1-17/18.[citado 2024 set. 15 ]

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