ReP USP - Resultado da busca

Artigo de periodico
Dynamics of the 3/1 planetary mean-motion resonance: an application to the HD60532 b-c planetary system (2016)
Alves, A. J; Michtchenko, Tatiana Alexandrovna; Santos, M. Tadeu dos
Source: Celestial Mechanics & Dinamical Astronomy. Unidade: IAG
Subjects: PLANETAS, DINÂMICA
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ABNT
ALVES, A. J e MICHTCHENKO, Tatiana Alexandrovna e SANTOS, M. Tadeu dos. Dynamics of the 3/1 planetary mean-motion resonance: an application to the HD60532 b-c planetary system. Celestial Mechanics & Dinamical Astronomy, v. 124, p. 311-334, 2016Tradução . . Disponível em: https://doi.org/10.1007/s10569-015-9664-x. Acesso em: 09 out. 2024.
APA
Alves, A. J., Michtchenko, T. A., & Santos, M. T. dos. (2016). Dynamics of the 3/1 planetary mean-motion resonance: an application to the HD60532 b-c planetary system. Celestial Mechanics & Dinamical Astronomy, 124, 311-334. doi:10.1007/s10569-015-9664-x
NLM
Alves AJ, Michtchenko TA, Santos MT dos. Dynamics of the 3/1 planetary mean-motion resonance: an application to the HD60532 b-c planetary system [Internet]. Celestial Mechanics & Dinamical Astronomy. 2016 ;124 311-334.[citado 2024 out. 09 ] Available from: https://doi.org/10.1007/s10569-015-9664-x
Vancouver
Alves AJ, Michtchenko TA, Santos MT dos. Dynamics of the 3/1 planetary mean-motion resonance: an application to the HD60532 b-c planetary system [Internet]. Celestial Mechanics & Dinamical Astronomy. 2016 ;124 311-334.[citado 2024 out. 09 ] Available from: https://doi.org/10.1007/s10569-015-9664-x
Artigo de periodico
FORS2/VLT survey of Milky Way globular clusters: II. Fe and Mg abundances of 51 Milky Way globular clusters on a homogeneous scale (2016)
Dias, B; Barbuy, Beatriz Leonor Silveira; Saviane, I; Held, E. V; Da Costa, G. S; Ortolani, S; Gullieuszik, M; Vásquez, S
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, DINÂMICA, CINEMÁTICA, POPULAÇÕES ESTELARES, FORMAÇÃO E EVOLUÇÃO DA GALÁXIA
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ABNT
DIAS, B et al. FORS2/VLT survey of Milky Way globular clusters: II. Fe and Mg abundances of 51 Milky Way globular clusters on a homogeneous scale. Astronomy & Astrophysics, v. 590, p. A9/1-A9/15, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201526765. Acesso em: 09 out. 2024.
APA
Dias, B., Barbuy, B. L. S., Saviane, I., Held, E. V., Da Costa, G. S., Ortolani, S., et al. (2016). FORS2/VLT survey of Milky Way globular clusters: II. Fe and Mg abundances of 51 Milky Way globular clusters on a homogeneous scale. Astronomy & Astrophysics, 590, A9/1-A9/15. doi:10.1051/0004-6361/201526765
NLM
Dias B, Barbuy BLS, Saviane I, Held EV, Da Costa GS, Ortolani S, Gullieuszik M, Vásquez S. FORS2/VLT survey of Milky Way globular clusters: II. Fe and Mg abundances of 51 Milky Way globular clusters on a homogeneous scale [Internet]. Astronomy & Astrophysics. 2016 ; 590 A9/1-A9/15.[citado 2024 out. 09 ] Available from: https://doi.org/10.1051/0004-6361/201526765
Vancouver
Dias B, Barbuy BLS, Saviane I, Held EV, Da Costa GS, Ortolani S, Gullieuszik M, Vásquez S. FORS2/VLT survey of Milky Way globular clusters: II. Fe and Mg abundances of 51 Milky Way globular clusters on a homogeneous scale [Internet]. Astronomy & Astrophysics. 2016 ; 590 A9/1-A9/15.[citado 2024 out. 09 ] Available from: https://doi.org/10.1051/0004-6361/201526765
Artigo de periodico
Secular dynamics of S-type planetary orbits in binary star systems: applicability domains of first- and second-order theories (2016)
Andrade-Ines, Eduardo; Beauge, Cristian; Michtchenco, Tatiana Alexandrovna; Robutel, Philippe
Source: Celestial Mechanics & Dynamical Astronomy. Unidade: IAG
Subjects: ESTRELAS BINÁRIAS, PLANETAS, DINÂMICA
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ABNT
ANDRADE-INES, Eduardo et al. Secular dynamics of S-type planetary orbits in binary star systems: applicability domains of first- and second-order theories. Celestial Mechanics & Dynamical Astronomy, v. 124, p. 405-432, 2016Tradução . . Disponível em: https://doi.org/10.1007/s10569-015-9669-5. Acesso em: 09 out. 2024.
APA
Andrade-Ines, E., Beauge, C., Michtchenco, T. A., & Robutel, P. (2016). Secular dynamics of S-type planetary orbits in binary star systems: applicability domains of first- and second-order theories. Celestial Mechanics & Dynamical Astronomy, 124, 405-432. doi:10.1007/s10569-015-9669-5
NLM
Andrade-Ines E, Beauge C, Michtchenco TA, Robutel P. Secular dynamics of S-type planetary orbits in binary star systems: applicability domains of first- and second-order theories [Internet]. Celestial Mechanics & Dynamical Astronomy. 2016 ; 124 405-432.[citado 2024 out. 09 ] Available from: https://doi.org/10.1007/s10569-015-9669-5
Vancouver
Andrade-Ines E, Beauge C, Michtchenco TA, Robutel P. Secular dynamics of S-type planetary orbits in binary star systems: applicability domains of first- and second-order theories [Internet]. Celestial Mechanics & Dynamical Astronomy. 2016 ; 124 405-432.[citado 2024 out. 09 ] Available from: https://doi.org/10.1007/s10569-015-9669-5
Artigo de periodico
FORS2/VLT survey of Milky Way globular clusters: I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8 (2015)
Dias, B; Barbuy, Beatriz Leonor Silveira; Saviane, I; Held, E. V; Costa, G. S. da; Ortolani, S; Vásquez, S; Gullieuszik, M; Katz, D
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR, CINEMÁTICA, DINÂMICA, POPULAÇÕES ESTELARES, GALÁXIA (VIA LÁCTEA)
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ABNT
DIAS, B et al. FORS2/VLT survey of Milky Way globular clusters: I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8. Astronomy & Astrophysics, v. 573, p. A13/1-A13/23, 2015Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201423996. Acesso em: 09 out. 2024.
APA
Dias, B., Barbuy, B. L. S., Saviane, I., Held, E. V., Costa, G. S. da, Ortolani, S., et al. (2015). FORS2/VLT survey of Milky Way globular clusters: I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8. Astronomy & Astrophysics, 573, A13/1-A13/23. doi:10.1051/0004-6361/201423996
NLM
Dias B, Barbuy BLS, Saviane I, Held EV, Costa GS da, Ortolani S, Vásquez S, Gullieuszik M, Katz D. FORS2/VLT survey of Milky Way globular clusters: I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8 [Internet]. Astronomy & Astrophysics. 2015 ; 573 A13/1-A13/23.[citado 2024 out. 09 ] Available from: https://doi.org/10.1051/0004-6361/201423996
Vancouver
Dias B, Barbuy BLS, Saviane I, Held EV, Costa GS da, Ortolani S, Vásquez S, Gullieuszik M, Katz D. FORS2/VLT survey of Milky Way globular clusters: I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8 [Internet]. Astronomy & Astrophysics. 2015 ; 573 A13/1-A13/23.[citado 2024 out. 09 ] Available from: https://doi.org/10.1051/0004-6361/201423996
Artigo de periodico
2.5D global-disk oscillation models of the Be shell star 'dzeta' Tauri: I. Spectroscopic and polarimetric analysis (2015)
Escolano, C; Carciofi, Alex Cavaliéri; Okazaki, A. T; Rivinius, T; Baade, D; Štefl,S
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: 09 out. 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 out. 09 ] 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 out. 09 ] Available from: https://doi.org/10.1051/0004-6361/201425446
Artigo de periodico
Formation and evolution of the two 4/3 resonant giants planets in HD 200964 (2015)
Tadeu dos Santos, M; Correa-Otto, J. A; Michtchenko, Tatiana Alexandrovna; Ferraz-Mello, Sylvio
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: PLANETAS (FORMAÇÃO), SATÉLITES (FORMAÇÃO), DINÂMICA, MECÂNICA CELESTE
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ABNT
TADEU DOS SANTOS, M et al. Formation and evolution of the two 4/3 resonant giants planets in HD 200964. Astronomy & Astrophysics, v. 573, p. A94/1-A94/15, 2015Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201424820. Acesso em: 09 out. 2024.
APA
Tadeu dos Santos, M., Correa-Otto, J. A., Michtchenko, T. A., & Ferraz-Mello, S. (2015). Formation and evolution of the two 4/3 resonant giants planets in HD 200964. Astronomy & Astrophysics, 573, A94/1-A94/15. doi:10.1051/0004-6361/201424820
NLM
Tadeu dos Santos M, Correa-Otto JA, Michtchenko TA, Ferraz-Mello S. Formation and evolution of the two 4/3 resonant giants planets in HD 200964 [Internet]. Astronomy & Astrophysics. 2015 ; 573 A94/1-A94/15.[citado 2024 out. 09 ] Available from: https://doi.org/10.1051/0004-6361/201424820
Vancouver
Tadeu dos Santos M, Correa-Otto JA, Michtchenko TA, Ferraz-Mello S. Formation and evolution of the two 4/3 resonant giants planets in HD 200964 [Internet]. Astronomy & Astrophysics. 2015 ; 573 A94/1-A94/15.[citado 2024 out. 09 ] Available from: https://doi.org/10.1051/0004-6361/201424820
Trabalho de evento-resumo periodico
The use of the Mathematica software in the study of planetary dynamics (2014)
Aguero, N. F; Michtchenko, Tatiana Alexandrovna
Source: Revista Mexicana de Astronomía y Astrofísica. Serie de Conferencias. Conference titles: Latin American Regional IAU Meeting. Unidade: IAG
Subjects: PLANETAS, DINÂMICA, SOFTWARES
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ABNT
AGUERO, N. F e MICHTCHENKO, Tatiana Alexandrovna. The use of the Mathematica software in the study of planetary dynamics. Revista Mexicana de Astronomía y Astrofísica. Serie de Conferencias. México: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. . Acesso em: 09 out. 2024. , 2014
APA
Aguero, N. F., & Michtchenko, T. A. (2014). The use of the Mathematica software in the study of planetary dynamics. Revista Mexicana de Astronomía y Astrofísica. Serie de Conferencias. México: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo.
NLM
Aguero NF, Michtchenko TA. The use of the Mathematica software in the study of planetary dynamics. Revista Mexicana de Astronomía y Astrofísica. Serie de Conferencias. 2014 ;[citado 2024 out. 09 ]
Vancouver
Aguero NF, Michtchenko TA. The use of the Mathematica software in the study of planetary dynamics. Revista Mexicana de Astronomía y Astrofísica. Serie de Conferencias. 2014 ;[citado 2024 out. 09 ]
Trabalho de evento-resumo
Dynamics of the 3:1 resonant planetary systems (2013)
Alves, Alan; Michtchenko, Tatiana Alexandrovna
Source: DDA Meeting 44. Conference titles: Meeting of the Division on Dynamical Astronomy. Unidade: IAG
Subjects: PLANETAS, DINÂMICA, MECÂNICA CELESTE
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ABNT
ALVES, Alan e MICHTCHENKO, Tatiana Alexandrovna. Dynamics of the 3:1 resonant planetary systems. 2013, Anais.. Washington: American Astronomical Society, 2013. . Acesso em: 09 out. 2024.
APA
Alves, A., & Michtchenko, T. A. (2013). Dynamics of the 3:1 resonant planetary systems. In DDA Meeting 44. Washington: American Astronomical Society.
NLM
Alves A, Michtchenko TA. Dynamics of the 3:1 resonant planetary systems. DDA Meeting 44. 2013 ;[citado 2024 out. 09 ]
Vancouver
Alves A, Michtchenko TA. Dynamics of the 3:1 resonant planetary systems. DDA Meeting 44. 2013 ;[citado 2024 out. 09 ]
Trabalho de evento-resumo
Determination of dynamical and physical parameters of the system CoRoT 3 (2013)
Tadeu dos Santos, Marcos; Ferraz-Mello, Sylvio; Michtchenko, Tatiana Alexandrovna
Source: DDA Meeting 44. Conference titles: Meeting of the Division on Dynamical Astronomy. Unidade: IAG
Subjects: PLANETAS, DINÂMICA, MECÂNICA CELESTE
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ABNT
TADEU DOS SANTOS, Marcos e FERRAZ-MELLO, Sylvio e MICHTCHENKO, Tatiana Alexandrovna. Determination of dynamical and physical parameters of the system CoRoT 3. 2013, Anais.. Washington: American Astronomical Society, 2013. . Acesso em: 09 out. 2024.
APA
Tadeu dos Santos, M., Ferraz-Mello, S., & Michtchenko, T. A. (2013). Determination of dynamical and physical parameters of the system CoRoT 3. In DDA Meeting 44. Washington: American Astronomical Society.
NLM
Tadeu dos Santos M, Ferraz-Mello S, Michtchenko TA. Determination of dynamical and physical parameters of the system CoRoT 3. DDA Meeting 44. 2013 ;[citado 2024 out. 09 ]
Vancouver
Tadeu dos Santos M, Ferraz-Mello S, Michtchenko TA. Determination of dynamical and physical parameters of the system CoRoT 3. DDA Meeting 44. 2013 ;[citado 2024 out. 09 ]
Trabalho de evento-resumo
Use of Mathematica software in the study of planetary dynamics (2013)
Aguero, Natasha Fioretto; Michtchenko, Tatiana Alexandrovna
Source: LARIM 2013: Abstract Book. Conference titles: Latin American Regional IAU Meeting. Unidade: IAG
Subjects: PLANETAS, DINÂMICA, SOFTWARES
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ABNT
AGUERO, Natasha Fioretto e MICHTCHENKO, Tatiana Alexandrovna. Use of Mathematica software in the study of planetary dynamics. 2013, Anais.. Paris: International Astronomical Union, 2013. . Acesso em: 09 out. 2024.
APA
Aguero, N. F., & Michtchenko, T. A. (2013). Use of Mathematica software in the study of planetary dynamics. In LARIM 2013: Abstract Book. Paris: International Astronomical Union.
NLM
Aguero NF, Michtchenko TA. Use of Mathematica software in the study of planetary dynamics. LARIM 2013: Abstract Book. 2013 ;[citado 2024 out. 09 ]
Vancouver
Aguero NF, Michtchenko TA. Use of Mathematica software in the study of planetary dynamics. LARIM 2013: Abstract Book. 2013 ;[citado 2024 out. 09 ]
Artigo de periodico-carta/editorial
Advances in theories and observations of solar system dynamics - II. [Preface] (2013)
Jatenco Pereira, Vera (Editor)
Source: Advances in Space Research. Unidade: IAG
Subjects: SISTEMA SOLAR, DINÂMICA
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ABNT
Advances in theories and observations of solar system dynamics - II. [Preface]. Advances in Space Research. Oxford: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. Disponível em: https://doi.org/10.1016/j.asr.2013.02.017. Acesso em: 09 out. 2024. , 2013
APA
Advances in theories and observations of solar system dynamics - II. [Preface]. (2013). Advances in theories and observations of solar system dynamics - II. [Preface]. Advances in Space Research. Oxford: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. doi:10.1016/j.asr.2013.02.017
NLM
Advances in theories and observations of solar system dynamics - II. [Preface] [Internet]. Advances in Space Research. 2013 ; 51 1809.[citado 2024 out. 09 ] Available from: https://doi.org/10.1016/j.asr.2013.02.017
Vancouver
Advances in theories and observations of solar system dynamics - II. [Preface] [Internet]. Advances in Space Research. 2013 ; 51 1809.[citado 2024 out. 09 ] Available from: https://doi.org/10.1016/j.asr.2013.02.017
Artigo de periodico
A kinematic study and membership analysis of the Lupus star-forming region (2013)
Galli, P. A. B; Bertout, C; Teixeira, Ramachrisna; Ducourant, C
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: DISTÂNCIAS ESTELARES, ESTRELAS, DINÂMICA, ASTROFÍSICA ESTELAR
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ABNT
GALLI, P. A. B et al. A kinematic study and membership analysis of the Lupus star-forming region. Astronomy & Astrophysics, v. 558, p. A77/1-A77/21, 2013Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201220704. Acesso em: 09 out. 2024.
APA
Galli, P. A. B., Bertout, C., Teixeira, R., & Ducourant, C. (2013). A kinematic study and membership analysis of the Lupus star-forming region. Astronomy & Astrophysics, 558, A77/1-A77/21. doi:10.1051/0004-6361/201220704
NLM
Galli PAB, Bertout C, Teixeira R, Ducourant C. A kinematic study and membership analysis of the Lupus star-forming region [Internet]. Astronomy & Astrophysics. 2013 ; 558 A77/1-A77/21.[citado 2024 out. 09 ] Available from: https://doi.org/10.1051/0004-6361/201220704
Vancouver
Galli PAB, Bertout C, Teixeira R, Ducourant C. A kinematic study and membership analysis of the Lupus star-forming region [Internet]. Astronomy & Astrophysics. 2013 ; 558 A77/1-A77/21.[citado 2024 out. 09 ] Available from: https://doi.org/10.1051/0004-6361/201220704
Trabalho de evento
Dynamical maps of the inner asteroid belt (2010)
Michtchenko, Tatiana Alexandrovna; Lazzaro, Daniela; Carvano, Jorge M; Ferraz-Mello, Sylvio
Source: Icy bodies of the Solar System. Proceedings. Conference titles: IAU Symposium. Unidade: IAG
Subjects: PLANETAS MENORES, ASTEROIDES, DINÂMICA
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ABNT
MICHTCHENKO, Tatiana Alexandrovna et al. Dynamical maps of the inner asteroid belt. 2010, Anais.. Cambridge: Cambridge University Press, 2010. . Acesso em: 09 out. 2024.
APA
Michtchenko, T. A., Lazzaro, D., Carvano, J. M., & Ferraz-Mello, S. (2010). Dynamical maps of the inner asteroid belt. In Icy bodies of the Solar System. Proceedings. Cambridge: Cambridge University Press.
NLM
Michtchenko TA, Lazzaro D, Carvano JM, Ferraz-Mello S. Dynamical maps of the inner asteroid belt. Icy bodies of the Solar System. Proceedings. 2010 ;[citado 2024 out. 09 ]
Vancouver
Michtchenko TA, Lazzaro D, Carvano JM, Ferraz-Mello S. Dynamical maps of the inner asteroid belt. Icy bodies of the Solar System. Proceedings. 2010 ;[citado 2024 out. 09 ]

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