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  • Source: Understanding extraterrestrial molecular complexity through experiments and observations. Conference titles: International Symposium and Workshop on Astrochemistry. Unidade: IAG

    Subjects: MEIO INTERESTELAR, FORMAÇÃO DE ESTRELAS

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      GAMA, D et al. Ionization-driven star formation:: the case IR bubble N10. 2016, Anais.. Campinas, SP: UNIVAP, 2016. . Acesso em: 20 out. 2024.
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      Gama, D., Lépine, J. R. D., Lefloch, B., & Mendonza, E. (2016). Ionization-driven star formation:: the case IR bubble N10. In Understanding extraterrestrial molecular complexity through experiments and observations. Campinas, SP: UNIVAP.
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      Gama D, Lépine JRD, Lefloch B, Mendonza E. Ionization-driven star formation:: the case IR bubble N10. Understanding extraterrestrial molecular complexity through experiments and observations. 2016 ;[citado 2024 out. 20 ]
    • Vancouver

      Gama D, Lépine JRD, Lefloch B, Mendonza E. Ionization-driven star formation:: the case IR bubble N10. Understanding extraterrestrial molecular complexity through experiments and observations. 2016 ;[citado 2024 out. 20 ]
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ASTROQUÍMICA, FORMAÇÃO DE ESTRELAS, MEIO INTERESTELAR, ABUNDÂNCIAS (ASTRONOMIA), JATOS (ASTRONOMIA)

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      LEFLOCH, Bertrand et al. Phosphorus-bearing molecules in solar-type star-forming regions: first PO detection. Monthly Notices of the Royal Astronomical Society, v. 462, p. 3937-3944, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw1918. Acesso em: 20 out. 2024.
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      Lefloch, B., Vastel, C., Viti, S., Jimenez-Serra, I., Codella, C., Podio, I., et al. (2016). Phosphorus-bearing molecules in solar-type star-forming regions: first PO detection. Monthly Notices of the Royal Astronomical Society, 462, 3937-3944. doi:10.1093/mnras/stw1918
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      Lefloch B, Vastel C, Viti S, Jimenez-Serra I, Codella C, Podio I, Ceccarelli C, Mendonza E, Lépine JRD, Bachiller R. Phosphorus-bearing molecules in solar-type star-forming regions: first PO detection [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 462 3937-3944.[citado 2024 out. 20 ] Available from: https://doi.org/10.1093/mnras/stw1918
    • Vancouver

      Lefloch B, Vastel C, Viti S, Jimenez-Serra I, Codella C, Podio I, Ceccarelli C, Mendonza E, Lépine JRD, Bachiller R. Phosphorus-bearing molecules in solar-type star-forming regions: first PO detection [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 462 3937-3944.[citado 2024 out. 20 ] Available from: https://doi.org/10.1093/mnras/stw1918
  • Source: Nature Communications. Unidade: IAG

    Subjects: GEOQUÍMICA, NEOPROTEROZOICO, OCEANOS

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      SANSJOFRE, Pierre et al. Multiple sulfur isotope evidence for massive oceanic sulfate depletion in the aftermath of Snowball Earth. Nature Communications, v. 7, p. 12192/1-12192/5, 2016Tradução . . Disponível em: https://doi.org/10.1038/ncomms12192. Acesso em: 20 out. 2024.
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      Sansjofre, P., Cartigny, P., Trindade, R. I. F. da, Nogueira, A. C. R., Agrinier, P., & Ader, M. (2016). Multiple sulfur isotope evidence for massive oceanic sulfate depletion in the aftermath of Snowball Earth. Nature Communications, 7, 12192/1-12192/5. doi:10.1038/ncomms12192
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      Sansjofre P, Cartigny P, Trindade RIF da, Nogueira ACR, Agrinier P, Ader M. Multiple sulfur isotope evidence for massive oceanic sulfate depletion in the aftermath of Snowball Earth [Internet]. Nature Communications. 2016 ; 7 12192/1-12192/5.[citado 2024 out. 20 ] Available from: https://doi.org/10.1038/ncomms12192
    • Vancouver

      Sansjofre P, Cartigny P, Trindade RIF da, Nogueira ACR, Agrinier P, Ader M. Multiple sulfur isotope evidence for massive oceanic sulfate depletion in the aftermath of Snowball Earth [Internet]. Nature Communications. 2016 ; 7 12192/1-12192/5.[citado 2024 out. 20 ] Available from: https://doi.org/10.1038/ncomms12192
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ABUNDÂNCIAS (ASTRONOMIA), ESTRELAS, ESPECTROSCOPIA

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      THYGESEN, A. O et al. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios. Astronomy & Astrophysics, v. 588, p. A66, 2016Tradução . . Disponível em: https://arxiv.org/pdf/1602.00058.pdf. Acesso em: 20 out. 2024.
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      Thygesen, A. O., Sbordone, L., Ludwig, H. -G., Ventura, P., Yong, D., Collet, R., et al. (2016). The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios. Astronomy & Astrophysics, 588, A66. doi:10.1051/0004-6361/201526643
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      Thygesen AO, Sbordone L, Ludwig H-G, Ventura P, Yong D, Collet R, Christlieb N, Moreno JLM, Zaggia S. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios [Internet]. Astronomy & Astrophysics. 2016 ; 588 A66.[citado 2024 out. 20 ] Available from: https://arxiv.org/pdf/1602.00058.pdf
    • Vancouver

      Thygesen AO, Sbordone L, Ludwig H-G, Ventura P, Yong D, Collet R, Christlieb N, Moreno JLM, Zaggia S. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios [Internet]. Astronomy & Astrophysics. 2016 ; 588 A66.[citado 2024 out. 20 ] Available from: https://arxiv.org/pdf/1602.00058.pdf
  • Source: Frontiers in the Earth Sciences. Unidade: IAG

    Subjects: NEOPROTEROZOICO, MAGNETISMO, RODÍNIA

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      MACOUIN, Melina et al. Response: Commentary: Is the Neoproterozoic oxygen burst a supercontinent legacy?. Frontiers in the Earth Sciences, v. 4, p. 83/1-83/3, 2016Tradução . . Disponível em: https://doi.org/10.3389/feart.2016.00083. Acesso em: 20 out. 2024.
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      Macouin, M., Rousse, S., Ganne, J., Denèle, Y., Roques, D., & Trindade, R. I. F. da. (2016). Response: Commentary: Is the Neoproterozoic oxygen burst a supercontinent legacy? Frontiers in the Earth Sciences, 4, 83/1-83/3. doi:10.3389/feart.2016.00083
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      Macouin M, Rousse S, Ganne J, Denèle Y, Roques D, Trindade RIF da. Response: Commentary: Is the Neoproterozoic oxygen burst a supercontinent legacy? [Internet]. Frontiers in the Earth Sciences. 2016 ; 4 83/1-83/3.[citado 2024 out. 20 ] Available from: https://doi.org/10.3389/feart.2016.00083
    • Vancouver

      Macouin M, Rousse S, Ganne J, Denèle Y, Roques D, Trindade RIF da. Response: Commentary: Is the Neoproterozoic oxygen burst a supercontinent legacy? [Internet]. Frontiers in the Earth Sciences. 2016 ; 4 83/1-83/3.[citado 2024 out. 20 ] Available from: https://doi.org/10.3389/feart.2016.00083
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ESTRELAS, INSTRUMENTAÇÃO (ASTRONOMIA), CAMPO MAGNÉTICO

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      WADE, G. A et al. The MiMeS survey of magnetism in massive stars: introduction and overview. Monthly Notices of the Royal Astronomical Society, v. 456, p. 2-22, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stv2568. Acesso em: 20 out. 2024.
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      Wade, G. A., Neiner, C., Alecian, E., & Carciofi, A. C. (2016). The MiMeS survey of magnetism in massive stars: introduction and overview. Monthly Notices of the Royal Astronomical Society, 456, 2-22. doi:10.1093/mnras/stv2568
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      Wade GA, Neiner C, Alecian E, Carciofi AC. The MiMeS survey of magnetism in massive stars: introduction and overview [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 456 2-22.[citado 2024 out. 20 ] Available from: https://doi.org/10.1093/mnras/stv2568
    • Vancouver

      Wade GA, Neiner C, Alecian E, Carciofi AC. The MiMeS survey of magnetism in massive stars: introduction and overview [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 456 2-22.[citado 2024 out. 20 ] Available from: https://doi.org/10.1093/mnras/stv2568
  • Source: Atmospheric Enviroment. Unidade: IAG

    Subjects: HIDROCARBONOS, ÁREAS METROPOLITANAS, POLUIÇÃO ATMOSFÉRICA, BIOCOMBUSTÍVEIS

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      DOMINUTTI, Pamela A et al. One-year of NMHCs hourly observations in São Paulo megacity: meteorological and traffic emissions effects in a large ethanol burning context. Atmospheric Enviroment, v. 142, p. 371-382, 2016Tradução . . Disponível em: https://doi.org/10.1016/j.atmosenv.2016.08.008. Acesso em: 20 out. 2024.
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      Dominutti, P. A., Nogueira, T., Borbon, A., Andrade, M. de F., & Fornaro, A. (2016). One-year of NMHCs hourly observations in São Paulo megacity: meteorological and traffic emissions effects in a large ethanol burning context. Atmospheric Enviroment, 142, 371-382. doi:10.1016/j.atmosenv.2016.08.008
    • NLM

      Dominutti PA, Nogueira T, Borbon A, Andrade M de F, Fornaro A. One-year of NMHCs hourly observations in São Paulo megacity: meteorological and traffic emissions effects in a large ethanol burning context [Internet]. Atmospheric Enviroment. 2016 ; 142 371-382.[citado 2024 out. 20 ] Available from: https://doi.org/10.1016/j.atmosenv.2016.08.008
    • Vancouver

      Dominutti PA, Nogueira T, Borbon A, Andrade M de F, Fornaro A. One-year of NMHCs hourly observations in São Paulo megacity: meteorological and traffic emissions effects in a large ethanol burning context [Internet]. Atmospheric Enviroment. 2016 ; 142 371-382.[citado 2024 out. 20 ] Available from: https://doi.org/10.1016/j.atmosenv.2016.08.008
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, CENTRO GALÁCTICO

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      BARBUY, Beatriz Leonor Silveira et al. High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP1. Astronomy & Astrophysics, v. 591, p. A53/1-A53/14, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201628106. Acesso em: 20 out. 2024.
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      Barbuy, B. L. S., Cantelli, E., Vemado, A., Ernandes, H., Ortoloni, S., Saviane, I., et al. (2016). High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP1. Astronomy & Astrophysics, 591, A53/1-A53/14. doi:10.1051/0004-6361/201628106
    • NLM

      Barbuy BLS, Cantelli E, Vemado A, Ernandes H, Ortoloni S, Saviane I, Bica E, Minniti D, Dias B, Momany Y, Hill V, Zoccali M, Siqueira Mello C. High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP1 [Internet]. Astronomy & Astrophysics. 2016 ;591 A53/1-A53/14.[citado 2024 out. 20 ] Available from: https://doi.org/10.1051/0004-6361/201628106
    • Vancouver

      Barbuy BLS, Cantelli E, Vemado A, Ernandes H, Ortoloni S, Saviane I, Bica E, Minniti D, Dias B, Momany Y, Hill V, Zoccali M, Siqueira Mello C. High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP1 [Internet]. Astronomy & Astrophysics. 2016 ;591 A53/1-A53/14.[citado 2024 out. 20 ] Available from: https://doi.org/10.1051/0004-6361/201628106
  • Source: Astrophysical Journal Supplement Series. Unidade: IAG

    Subjects: ESTRELAS, EVOLUÇÃO ESTELAR

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      ACERO, F et al. The first fermi lat supernova remnant catalog. Astrophysical Journal Supplement Series, 2016Tradução . . Disponível em: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0067-0049/224/1/8/pdf. Acesso em: 20 out. 2024.
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      Acero, F., Ackermann, M., Ajello, M., & Silva, R. N. da. (2016). The first fermi lat supernova remnant catalog. Astrophysical Journal Supplement Series. doi:10.3847/0067-0049/224/1/8
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      Acero F, Ackermann M, Ajello M, Silva RN da. The first fermi lat supernova remnant catalog [Internet]. Astrophysical Journal Supplement Series. 2016 ;[citado 2024 out. 20 ] Available from: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0067-0049/224/1/8/pdf
    • Vancouver

      Acero F, Ackermann M, Ajello M, Silva RN da. The first fermi lat supernova remnant catalog [Internet]. Astrophysical Journal Supplement Series. 2016 ;[citado 2024 out. 20 ] Available from: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0067-0049/224/1/8/pdf
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: AGLOMERADOS DE GALÁXIAS, COSMOLOGIA, MATÉRIA ESCURA, ESTRUTURA DO UNIVERSO

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      ASCASO , B et al. An accurate cluster selection function for the J-PAS narrow-band wide-field survey. Monthly Notices of the Royal Astronomical Society, v. 456, p. 4291-4304, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stv2988. Acesso em: 20 out. 2024.
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      Ascaso , B., Benítez, N., Dupke, R., Cypriano, E. S., Lima Neto, G. C. B., López-Sanjuan, C., et al. (2016). An accurate cluster selection function for the J-PAS narrow-band wide-field survey. Monthly Notices of the Royal Astronomical Society, 456, 4291-4304. doi:10.1093/mnras/stv2988
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      Ascaso B, Benítez N, Dupke R, Cypriano ES, Lima Neto GCB, López-Sanjuan C, Varela J, Alcaniz JS, Broadhurst T, Cenarro AJ, Chandrachani Devi N, Díaz-García LA, Fernandes CA, Hernández-Monteagudo C, Mei S, Mendes de Oliveira CL, Molino A, Oteo I, Schoenell W, Sodré Júnior L, Viironen K, Marín F. An accurate cluster selection function for the J-PAS narrow-band wide-field survey [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 456 4291-4304.[citado 2024 out. 20 ] Available from: https://doi.org/10.1093/mnras/stv2988
    • Vancouver

      Ascaso B, Benítez N, Dupke R, Cypriano ES, Lima Neto GCB, López-Sanjuan C, Varela J, Alcaniz JS, Broadhurst T, Cenarro AJ, Chandrachani Devi N, Díaz-García LA, Fernandes CA, Hernández-Monteagudo C, Mei S, Mendes de Oliveira CL, Molino A, Oteo I, Schoenell W, Sodré Júnior L, Viironen K, Marín F. An accurate cluster selection function for the J-PAS narrow-band wide-field survey [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 456 4291-4304.[citado 2024 out. 20 ] Available from: https://doi.org/10.1093/mnras/stv2988
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, GALÁXIA (VIA LÁCTEA)

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      VAN DER SWAELMEN, M et al. Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants. Astronomy & Astrophysics, v. 586, p. A1/1-A1/11, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201525709. Acesso em: 20 out. 2024.
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      van der Swaelmen, M., Barbuy, B. L. S., Hill, V., Zoccali, M., Minniti, D., Ortolani, S., & Gómez, A. (2016). Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants. Astronomy & Astrophysics, 586, A1/1-A1/11. doi:10.1051/0004-6361/201525709
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      van der Swaelmen M, Barbuy BLS, Hill V, Zoccali M, Minniti D, Ortolani S, Gómez A. Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants [Internet]. Astronomy & Astrophysics. 2016 ; 586 A1/1-A1/11.[citado 2024 out. 20 ] Available from: https://doi.org/10.1051/0004-6361/201525709
    • Vancouver

      van der Swaelmen M, Barbuy BLS, Hill V, Zoccali M, Minniti D, Ortolani S, Gómez A. Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants [Internet]. Astronomy & Astrophysics. 2016 ; 586 A1/1-A1/11.[citado 2024 out. 20 ] Available from: https://doi.org/10.1051/0004-6361/201525709
  • Source: Geophysical Journal International. Unidade: IAG

    Subjects: MAGNETISMO, PALEOMAGNETISMO (DATAÇÃO ARQUEOLÓGICA)

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      TERRA-NOVA, Filipe et al. Using archaeomagnetic field models to constrain the physics of the core: robustness and preferred locations of reversed flux patches. Geophysical Journal International, v. 206, p. 1890-1913, 2016Tradução . . Disponível em: https://doi.org/10.1093/gji/ggw248. Acesso em: 20 out. 2024.
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      Terra-Nova, F., Amit, H., Hartmann, G., & Trindade, R. I. F. da. (2016). Using archaeomagnetic field models to constrain the physics of the core: robustness and preferred locations of reversed flux patches. Geophysical Journal International, 206, 1890-1913. doi:10.1093/gji/ggw248
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      Terra-Nova F, Amit H, Hartmann G, Trindade RIF da. Using archaeomagnetic field models to constrain the physics of the core: robustness and preferred locations of reversed flux patches [Internet]. Geophysical Journal International. 2016 ; 206 1890-1913.[citado 2024 out. 20 ] Available from: https://doi.org/10.1093/gji/ggw248
    • Vancouver

      Terra-Nova F, Amit H, Hartmann G, Trindade RIF da. Using archaeomagnetic field models to constrain the physics of the core: robustness and preferred locations of reversed flux patches [Internet]. Geophysical Journal International. 2016 ; 206 1890-1913.[citado 2024 out. 20 ] Available from: https://doi.org/10.1093/gji/ggw248
  • Source: Understanding extraterrestrial molecular complexity through experiments and observations. Conference titles: International Symposium and Workshop on Astrochemistry. Unidade: IAG

    Subjects: ASTROFÍSICA ESTELAR, ABUNDÂNCIA ESTELAR

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      MENDOZA, Edgar et al. Dectection ofcyanopolyynes in the protostellar shock L1157-B1. 2016, Anais.. Campinas, SP: UNIVAP, 2016. . Acesso em: 20 out. 2024.
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      Mendoza, E., Lefloch, B., Lépine, J. R. D., Boechat-Roberty, H. M., & Bachiller, R. (2016). Dectection ofcyanopolyynes in the protostellar shock L1157-B1. In Understanding extraterrestrial molecular complexity through experiments and observations. Campinas, SP: UNIVAP.
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      Mendoza E, Lefloch B, Lépine JRD, Boechat-Roberty HM, Bachiller R. Dectection ofcyanopolyynes in the protostellar shock L1157-B1. Understanding extraterrestrial molecular complexity through experiments and observations. 2016 ;[citado 2024 out. 20 ]
    • Vancouver

      Mendoza E, Lefloch B, Lépine JRD, Boechat-Roberty HM, Bachiller R. Dectection ofcyanopolyynes in the protostellar shock L1157-B1. Understanding extraterrestrial molecular complexity through experiments and observations. 2016 ;[citado 2024 out. 20 ]
  • 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: 20 out. 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
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      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. 20 ] 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. 20 ] Available from: https://doi.org/10.1007/s10569-015-9669-5
  • Source: Journal of Physics: Conference Series. Conference titles: Nuclear Physics in Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIAS (ASTRONOMIA), ASTROFÍSICA ESTELAR

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      SIQUEIRA MELLO, C e SPITE, M e BARBUY, Beatriz Leonor Silveira. HST/STIS abundances in the uranium rich metal poor star CS 31082-001: constraints on the r-process. Journal of Physics: Conference Series. Bristol: Institute of Physics - IOP. Disponível em: http://iopscience.iop.org/article/10.1088/1742-6596/665/1/012056/pdf. Acesso em: 20 out. 2024. , 2016
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      Siqueira Mello, C., Spite, M., & Barbuy, B. L. S. (2016). HST/STIS abundances in the uranium rich metal poor star CS 31082-001: constraints on the r-process. Journal of Physics: Conference Series. Bristol: Institute of Physics - IOP. doi:10.1088/1742-6596/665/1/012056
    • NLM

      Siqueira Mello C, Spite M, Barbuy BLS. HST/STIS abundances in the uranium rich metal poor star CS 31082-001: constraints on the r-process [Internet]. Journal of Physics: Conference Series. 2016 ;665 012056.[citado 2024 out. 20 ] Available from: http://iopscience.iop.org/article/10.1088/1742-6596/665/1/012056/pdf
    • Vancouver

      Siqueira Mello C, Spite M, Barbuy BLS. HST/STIS abundances in the uranium rich metal poor star CS 31082-001: constraints on the r-process [Internet]. Journal of Physics: Conference Series. 2016 ;665 012056.[citado 2024 out. 20 ] Available from: http://iopscience.iop.org/article/10.1088/1742-6596/665/1/012056/pdf

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