Filtros : "PLANETAS" "IAG-AGA" Removidos: "Nunes, Maria Tereza" "IME-MAE" "1982" "Catelan, M" Limpar

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  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: PLANETAS, SATÉLITES, DISCOS DE ACRESÇÃO

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      DEPAULA, L. A e MICHTCHENKO, Tatiana Alexandrovna e SOUSA-SILVA, P. A. Adapting a solid accretion scenario for migrating planets in FARGO3D. Monthly Notices of the Royal Astronomical Society, v. 490, n. 2, p. 2336-2346, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz2762. Acesso em: 07 jun. 2024.
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      DePaula, L. A., Michtchenko, T. A., & Sousa-Silva, P. A. (2019). Adapting a solid accretion scenario for migrating planets in FARGO3D. Monthly Notices of the Royal Astronomical Society, 490( 2), 2336-2346. doi:10.1093/mnras/stz2762
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      DePaula LA, Michtchenko TA, Sousa-Silva PA. Adapting a solid accretion scenario for migrating planets in FARGO3D [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490( 2): 2336-2346.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1093/mnras/stz2762
    • Vancouver

      DePaula LA, Michtchenko TA, Sousa-Silva PA. Adapting a solid accretion scenario for migrating planets in FARGO3D [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490( 2): 2336-2346.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1093/mnras/stz2762
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: PLANETAS, SATÉLITES

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      DEPAULA, L. A e MICHTCHENKO, Tatiana Alexandrovna. Adapting a gas accretion scenario for migrating planets in FARGO3D. Monthly Notices of the Royal Astronomical Society, v. 483. 2, p. 1599-1608, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty3045. Acesso em: 07 jun. 2024.
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      DePaula, L. A., & Michtchenko, T. A. (2019). Adapting a gas accretion scenario for migrating planets in FARGO3D. Monthly Notices of the Royal Astronomical Society, 483. 2, 1599-1608. doi:10.1093/mnras/sty3045
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      DePaula LA, Michtchenko TA. Adapting a gas accretion scenario for migrating planets in FARGO3D [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 483. 2 1599-1608.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1093/mnras/sty3045
    • Vancouver

      DePaula LA, Michtchenko TA. Adapting a gas accretion scenario for migrating planets in FARGO3D [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 483. 2 1599-1608.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1093/mnras/sty3045
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDANCIA ESTELAR, PLANETAS

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      BOTELHO, Roberto et al. Thorium in solar twins: implications for habitability in rocky planets. Monthly Notices of the Royal Astronomical Society, v. 482, p. 1690-1700, 2019Tradução . . Disponível em: https://academic.oup.com/mnras/article/490/2/2448/5583050. Acesso em: 07 jun. 2024.
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      Botelho, R., Moreno, J. L. M., Alves-Brito, A., & Galarza, J. Y. (2019). Thorium in solar twins: implications for habitability in rocky planets. Monthly Notices of the Royal Astronomical Society, 482, 1690-1700. doi:10.1093/mnras/sty2791
    • NLM

      Botelho R, Moreno JLM, Alves-Brito A, Galarza JY. Thorium in solar twins: implications for habitability in rocky planets [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 482 1690-1700.[citado 2024 jun. 07 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
    • Vancouver

      Botelho R, Moreno JLM, Alves-Brito A, Galarza JY. Thorium in solar twins: implications for habitability in rocky planets [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 482 1690-1700.[citado 2024 jun. 07 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: PLANETAS, SATÉLITES

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      RODRÍGUEZ, A e CORREA-OTTO, J. A. Primordial migration of co-orbital satellites as a mechanism for the horseshoe orbit of Janus –Epimetheus. Monthly Notices of the Royal Astronomical Society, v. 487. 2, p. 1973-1979, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz1428. Acesso em: 07 jun. 2024.
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      Rodríguez, A., & Correa-Otto, J. A. (2019). Primordial migration of co-orbital satellites as a mechanism for the horseshoe orbit of Janus –Epimetheus. Monthly Notices of the Royal Astronomical Society, 487. 2, 1973-1979. doi:10.1093/mnras/stz1428
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      Rodríguez A, Correa-Otto JA. Primordial migration of co-orbital satellites as a mechanism for the horseshoe orbit of Janus –Epimetheus [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 487. 2 1973-1979.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1093/mnras/stz1428
    • Vancouver

      Rodríguez A, Correa-Otto JA. Primordial migration of co-orbital satellites as a mechanism for the horseshoe orbit of Janus –Epimetheus [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 487. 2 1973-1979.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1093/mnras/stz1428
  • Source: Astronomy and Astrophysysics. Unidade: IAG

    Subjects: PLANETAS, ABUNDÂNCIA ESTELAR

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      LORENZO-OLIVEIRA, Diego et al. The solar twin planet search: The age - chromospheric activity relation. Astronomy and Astrophysysics, v. 619, p. A73, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201629294. Acesso em: 07 jun. 2024.
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      Lorenzo-Oliveira, D., Freitas, F. C., Moreno, J. L. M., & Bedell, M. (2018). The solar twin planet search: The age - chromospheric activity relation. Astronomy and Astrophysysics, 619, A73. doi:10.1051/0004-6361/201629294
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      Lorenzo-Oliveira D, Freitas FC, Moreno JLM, Bedell M. The solar twin planet search: The age - chromospheric activity relation [Internet]. Astronomy and Astrophysysics. 2018 ;619 A73.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1051/0004-6361/201629294
    • Vancouver

      Lorenzo-Oliveira D, Freitas FC, Moreno JLM, Bedell M. The solar twin planet search: The age - chromospheric activity relation [Internet]. Astronomy and Astrophysysics. 2018 ;619 A73.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1051/0004-6361/201629294
  • Source: Astronomy and Astrophysysics. Unidade: IAG

    Subjects: PLANETAS, ABUNDÂNCIA ESTELAR

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      MORENO, Jorge Luiz Meléndez et al. The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468. Astronomy and Astrophysysics, v. 597, p. A34, 2017Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527775. Acesso em: 07 jun. 2024.
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      Moreno, J. L. M., Bedell, M., Bean, J. L., Mello, S. F., Galarza, J. Y., Santos, L. dos, et al. (2017). The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468. Astronomy and Astrophysysics, 597, A34. doi:10.1051/0004-6361/201527775
    • NLM

      Moreno JLM, Bedell M, Bean JL, Mello SF, Galarza JY, Santos L dos, Spina L, Maia MT. The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468 [Internet]. Astronomy and Astrophysysics. 2017 ;597 A34.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1051/0004-6361/201527775
    • Vancouver

      Moreno JLM, Bedell M, Bean JL, Mello SF, Galarza JY, Santos L dos, Spina L, Maia MT. The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468 [Internet]. Astronomy and Astrophysysics. 2017 ;597 A34.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1051/0004-6361/201527775
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, PLANETAS

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      BEDELL, Megan et al. Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization. Astrophysical Journal, v. 839, p. 94. 2017, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aa6a1d. Acesso em: 07 jun. 2024.
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      Bedell, M., Bean, J. L., Moreno, J. L. M., Mills, S. M., Fabrycky, D. C., Freitas, F. C., et al. (2017). Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization. Astrophysical Journal, 839, 94. 2017. doi:10.3847/1538-4357/aa6a1d
    • NLM

      Bedell M, Bean JL, Moreno JLM, Mills SM, Fabrycky DC, Freitas FC, Ramírez I, Asplund M, Liu F, Yong D. Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization [Internet]. Astrophysical Journal. 2017 ; 839 94. 2017.[citado 2024 jun. 07 ] Available from: https://doi.org/10.3847/1538-4357/aa6a1d
    • Vancouver

      Bedell M, Bean JL, Moreno JLM, Mills SM, Fabrycky DC, Freitas FC, Ramírez I, Asplund M, Liu F, Yong D. Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization [Internet]. Astrophysical Journal. 2017 ; 839 94. 2017.[citado 2024 jun. 07 ] Available from: https://doi.org/10.3847/1538-4357/aa6a1d
  • Source: Astrophysical Journal (Online). Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, PLANETAS

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      STORCHI-BERGMANN, Thaisa et al. Double-Peaked Profiles: Ubiquitous Signatures of Disks in the Broad Emission Lines of Active Galactic Nuclei. Astrophysical Journal (Online), v. 835, n. 2, p. 236, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/835/2/236. Acesso em: 07 jun. 2024.
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      Storchi-Bergmann, T., Schimoia, J. S., Peterson, B. M., Elvis, M., Denney, K. D., Eracleous, M., & Silva, R. N. da. (2017). Double-Peaked Profiles: Ubiquitous Signatures of Disks in the Broad Emission Lines of Active Galactic Nuclei. Astrophysical Journal (Online), 835( 2), 236. doi:10.3847/1538-4357/835/2/236
    • NLM

      Storchi-Bergmann T, Schimoia JS, Peterson BM, Elvis M, Denney KD, Eracleous M, Silva RN da. Double-Peaked Profiles: Ubiquitous Signatures of Disks in the Broad Emission Lines of Active Galactic Nuclei [Internet]. Astrophysical Journal (Online). 2017 ;835( 2): 236.[citado 2024 jun. 07 ] Available from: https://doi.org/10.3847/1538-4357/835/2/236
    • Vancouver

      Storchi-Bergmann T, Schimoia JS, Peterson BM, Elvis M, Denney KD, Eracleous M, Silva RN da. Double-Peaked Profiles: Ubiquitous Signatures of Disks in the Broad Emission Lines of Active Galactic Nuclei [Internet]. Astrophysical Journal (Online). 2017 ;835( 2): 236.[citado 2024 jun. 07 ] Available from: https://doi.org/10.3847/1538-4357/835/2/236
  • Source: ASTRONOMY & ASTROPHYSICS. Unidade: IAG

    Subjects: MECÂNICA CELESTE, PLANETAS

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      RODET, L. et al. Origin of the wide-orbit circumbinary giant planet HD-106906 - A dynamical scenario and its impact on the disk. ASTRONOMY & ASTROPHYSICS, v. 602, p. online, 2017Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201630269. Acesso em: 07 jun. 2024.
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      RODET, L., Beust, H., Bonnefoy, M., Lagrange, A. -M., Galli, P. A. B., DUCOURANT, C., & Teixeira, R. (2017). Origin of the wide-orbit circumbinary giant planet HD-106906 - A dynamical scenario and its impact on the disk. ASTRONOMY & ASTROPHYSICS, 602, online. doi:10.1051/0004-6361/201630269
    • NLM

      RODET L, Beust H, Bonnefoy M, Lagrange A-M, Galli PAB, DUCOURANT C, Teixeira R. Origin of the wide-orbit circumbinary giant planet HD-106906 - A dynamical scenario and its impact on the disk [Internet]. ASTRONOMY & ASTROPHYSICS. 2017 ;602 online.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1051/0004-6361/201630269
    • Vancouver

      RODET L, Beust H, Bonnefoy M, Lagrange A-M, Galli PAB, DUCOURANT C, Teixeira R. Origin of the wide-orbit circumbinary giant planet HD-106906 - A dynamical scenario and its impact on the disk [Internet]. ASTRONOMY & ASTROPHYSICS. 2017 ;602 online.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1051/0004-6361/201630269
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ESTRELAS, PLANETAS, GALÁXIA (VIA LÁCTEA), FORMAÇÃO E EVOLUÇÃO DA GALÁXIA

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      SPINA, Lorenzo e MORENO, Jorge Luiz Meléndez e RAMÍREZ, Iván. Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars. Astronomy & Astrophysics, v. 585, p. A152/1-A152/15, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527429. Acesso em: 07 jun. 2024.
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      Spina, L., Moreno, J. L. M., & Ramírez, I. (2016). Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars. Astronomy & Astrophysics, 585, A152/1-A152/15. doi:10.1051/0004-6361/201527429
    • NLM

      Spina L, Moreno JLM, Ramírez I. Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars [Internet]. Astronomy & Astrophysics. 2016 ; 585 A152/1-A152/15.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1051/0004-6361/201527429
    • Vancouver

      Spina L, Moreno JLM, Ramírez I. Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars [Internet]. Astronomy & Astrophysics. 2016 ; 585 A152/1-A152/15.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1051/0004-6361/201527429
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIAS SOLARES, ABUNDÂNCIA ESTELAR, TERRA (PLANETA), PLANETAS

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      GALARZA, Jhon Yana e MORENO, Jorge Luiz Meléndez e COHEN, Judith G. Serendipitous discovery of the faint solar twin Inti 1. Astronomy & Astrophysics, v. 589, p. A65/1-A65/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527477. Acesso em: 07 jun. 2024.
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      Galarza, J. Y., Moreno, J. L. M., & Cohen, J. G. (2016). Serendipitous discovery of the faint solar twin Inti 1. Astronomy & Astrophysics, 589, A65/1-A65/8. doi:10.1051/0004-6361/201527477
    • NLM

      Galarza JY, Moreno JLM, Cohen JG. Serendipitous discovery of the faint solar twin Inti 1 [Internet]. Astronomy & Astrophysics. 2016 ; 589 A65/1-A65/8.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1051/0004-6361/201527477
    • Vancouver

      Galarza JY, Moreno JLM, Cohen JG. Serendipitous discovery of the faint solar twin Inti 1 [Internet]. Astronomy & Astrophysics. 2016 ; 589 A65/1-A65/8.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1051/0004-6361/201527477
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: PLANETAS, SATÉLITES, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES

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      LIU, F et al. The Hyades open cluster is chemically inhomogeneous. Monthly Notices of the Royal Astronomical Society, v. 457, p. 3934-3948, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw247. Acesso em: 07 jun. 2024.
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      Liu, F., Yong, D., Asplund, M., Ramírez, I., & Moreno, J. L. M. (2016). The Hyades open cluster is chemically inhomogeneous. Monthly Notices of the Royal Astronomical Society, 457, 3934-3948. doi:10.1093/mnras/stw247
    • NLM

      Liu F, Yong D, Asplund M, Ramírez I, Moreno JLM. The Hyades open cluster is chemically inhomogeneous [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 457 3934-3948.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1093/mnras/stw247
    • Vancouver

      Liu F, Yong D, Asplund M, Ramírez I, Moreno JLM. The Hyades open cluster is chemically inhomogeneous [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 457 3934-3948.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1093/mnras/stw247
  • Source: Celestial Mechanics & Dinamical Astronomy. Unidade: IAG

    Subjects: PLANETAS, DINÂMICA

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      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: 07 jun. 2024.
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      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
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      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 jun. 07 ] 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 jun. 07 ] Available from: https://doi.org/10.1007/s10569-015-9664-x
  • Source: Revista Mexicana de Astronomíay Astrofísica. Unidade: IAG

    Subjects: ESPECTROSCOPIA, NEBULOSAS, PLANETAS, MEIO INTERESTELAR, MÉTODOS NUMÉRICOS

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      LAGO, P. J. A e COSTA, Roberto Dell'Aglio Dias da. NGC 2440: a morpho-kinematical model. Revista Mexicana de Astronomíay Astrofísica, v. 52, p. 329-337, 2016Tradução . . Disponível em: http://www.astroscu.unam.mx/rmaa/RMxAA.52-2/PDF/RMxAA.52-2_plago.pdf. Acesso em: 07 jun. 2024.
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      Lago, P. J. A., & Costa, R. D. 'A. D. da. (2016). NGC 2440: a morpho-kinematical model. Revista Mexicana de Astronomíay Astrofísica, 52, 329-337. Recuperado de http://www.astroscu.unam.mx/rmaa/RMxAA.52-2/PDF/RMxAA.52-2_plago.pdf
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      Lago PJA, Costa RD'AD da. NGC 2440: a morpho-kinematical model [Internet]. Revista Mexicana de Astronomíay Astrofísica. 2016 ; 52 329-337.[citado 2024 jun. 07 ] Available from: http://www.astroscu.unam.mx/rmaa/RMxAA.52-2/PDF/RMxAA.52-2_plago.pdf
    • Vancouver

      Lago PJA, Costa RD'AD da. NGC 2440: a morpho-kinematical model [Internet]. Revista Mexicana de Astronomíay Astrofísica. 2016 ; 52 329-337.[citado 2024 jun. 07 ] Available from: http://www.astroscu.unam.mx/rmaa/RMxAA.52-2/PDF/RMxAA.52-2_plago.pdf
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: PLANETAS, SATÉLITES, ABUNDÂNCIA ESTELAR, ESTRELAS

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      LIU, F et al. The detailed chemical composition of the terrestrial planet host Kepler-10. Monthly Notices of the Royal Astronomical Society, v. 456, p. 2636-2646, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stv2821. Acesso em: 07 jun. 2024.
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      Liu, F., Yong, D., Asplund, M., Ramírez, I., Moreno, J. L. M., Gustafsson, B., et al. (2016). The detailed chemical composition of the terrestrial planet host Kepler-10. Monthly Notices of the Royal Astronomical Society, 456, 2636-2646. doi:10.1093/mnras/stv2821
    • NLM

      Liu F, Yong D, Asplund M, Ramírez I, Moreno JLM, Gustafsson B, Howes MJ, Roederer IU, Lambert DL, Bensby T. The detailed chemical composition of the terrestrial planet host Kepler-10 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 456 2636-2646.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1093/mnras/stv2821
    • Vancouver

      Liu F, Yong D, Asplund M, Ramírez I, Moreno JLM, Gustafsson B, Howes MJ, Roederer IU, Lambert DL, Bensby T. The detailed chemical composition of the terrestrial planet host Kepler-10 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 456 2636-2646.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1093/mnras/stv2821
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIAS SOLARES, ABUNDÂNCIA ESTELAR, PLANETAS

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      GALARZA, Jhon Yana et al. High-precision analysis of the solar twin HIP 100963. Astronomy & Astrophysics, v. 589, p. A17/1-A17/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527912. Acesso em: 07 jun. 2024.
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      Galarza, J. Y., Moreno, J. L. M., Ramírez, I., Yong, D., Karakas, A. I., Asplund, M., & Liu, F. (2016). High-precision analysis of the solar twin HIP 100963. Astronomy & Astrophysics, 589, A17/1-A17/8. doi:10.1051/0004-6361/201527912
    • NLM

      Galarza JY, Moreno JLM, Ramírez I, Yong D, Karakas AI, Asplund M, Liu F. High-precision analysis of the solar twin HIP 100963 [Internet]. Astronomy & Astrophysics. 2016 ; 589 A17/1-A17/8.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1051/0004-6361/201527912
    • Vancouver

      Galarza JY, Moreno JLM, Ramírez I, Yong D, Karakas AI, Asplund M, Liu F. High-precision analysis of the solar twin HIP 100963 [Internet]. Astronomy & Astrophysics. 2016 ; 589 A17/1-A17/8.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1051/0004-6361/201527912
  • Source: Anais do CBDO2016: programação e resumos. Conference titles: Colóquio Brasileiro de Dinâmica Orbital. Unidade: IAG

    Subjects: PLANETAS, MECÂNICA CELESTE

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      PAULA, Luiz alberto de e MICHTCHENKO, Tatiana Alexandrovna. Elaboração de um cenário para formação de planetas gigantes. 2016, Anais.. Guaratinguetá: UNESP, 2016. . Acesso em: 07 jun. 2024.
    • APA

      Paula, L. alberto de, & Michtchenko, T. A. (2016). Elaboração de um cenário para formação de planetas gigantes. In Anais do CBDO2016: programação e resumos. Guaratinguetá: UNESP.
    • NLM

      Paula L alberto de, Michtchenko TA. Elaboração de um cenário para formação de planetas gigantes. Anais do CBDO2016: programação e resumos. 2016 ;[citado 2024 jun. 07 ]
    • Vancouver

      Paula L alberto de, Michtchenko TA. Elaboração de um cenário para formação de planetas gigantes. Anais do CBDO2016: programação e resumos. 2016 ;[citado 2024 jun. 07 ]
  • Source: Celestial Mechanics & Dynamical Astronomy. Unidade: IAG

    Subjects: ESTRELAS BINÁRIAS, PLANETAS, DINÂMICA

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      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: 07 jun. 2024.
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      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 jun. 07 ] 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 jun. 07 ] Available from: https://doi.org/10.1007/s10569-015-9669-5
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, EVOLUÇÃO ESTELAR, PLANETAS

    Acesso à fonteDOIHow to cite
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      CARLOS, Marília e NISSEN, Poul E e MORENO, Jorge Luiz Meléndez. Correlation between lithium abundances and ages of solar twin stars. Astronomy & Astrophysics, v. 587, p. A100/1-A100/6, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527478. Acesso em: 07 jun. 2024.
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      Carlos, M., Nissen, P. E., & Moreno, J. L. M. (2016). Correlation between lithium abundances and ages of solar twin stars. Astronomy & Astrophysics, 587, A100/1-A100/6. doi:10.1051/0004-6361/201527478
    • NLM

      Carlos M, Nissen PE, Moreno JLM. Correlation between lithium abundances and ages of solar twin stars [Internet]. Astronomy & Astrophysics. 2016 ; 587 A100/1-A100/6.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1051/0004-6361/201527478
    • Vancouver

      Carlos M, Nissen PE, Moreno JLM. Correlation between lithium abundances and ages of solar twin stars [Internet]. Astronomy & Astrophysics. 2016 ; 587 A100/1-A100/6.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1051/0004-6361/201527478
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: PLANETAS, SATÉLITES, ATIVIDADE ESTELAR, VELOCIDADE

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      BEDELL, M et al. The solar twin planet search: II. A Jupiter twin around a solar twin. Astronomy & Astrophysics, v. 581, p. A34/1-A34/7, 2015Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201525748. Acesso em: 07 jun. 2024.
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      Bedell, M., Moreno, J. L. M., Bean, J. L., Ramírez, I., Asplund, M., Alves-Brito, A., et al. (2015). The solar twin planet search: II. A Jupiter twin around a solar twin. Astronomy & Astrophysics, 581, A34/1-A34/7. doi:10.1051/0004-6361/201525748
    • NLM

      Bedell M, Moreno JLM, Bean JL, Ramírez I, Asplund M, Alves-Brito A, Casagrande L, Dreizler S, Monroe T, Spina L, Tucci Maia M. The solar twin planet search: II. A Jupiter twin around a solar twin [Internet]. Astronomy & Astrophysics. 2015 ; 581 A34/1-A34/7.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1051/0004-6361/201525748
    • Vancouver

      Bedell M, Moreno JLM, Bean JL, Ramírez I, Asplund M, Alves-Brito A, Casagrande L, Dreizler S, Monroe T, Spina L, Tucci Maia M. The solar twin planet search: II. A Jupiter twin around a solar twin [Internet]. Astronomy & Astrophysics. 2015 ; 581 A34/1-A34/7.[citado 2024 jun. 07 ] Available from: https://doi.org/10.1051/0004-6361/201525748

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