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Filtros : "IAU Symposium" "IAG" Removidos: "2013" "2022" "Financiamento AKA" "Financiamento CAPES" "Abstract Book" Limpar

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  • Trabalho de evento

    Gas outflow in Seyfert galaxies: 3D radiative cooling hydrodynamical simulations (2015)

    Melioli, Claudio; Dal Pino, Elisabete Maria de Gouveia

    Source: Proceedings IAU Symposium, 313: Extragalactic jets from every angle. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: GALÁXIAS SEY FERT, JATOS (ASTRONOMIA), HIDRODINÂMICA

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      MELIOLI, Claudio e DAL PINO, Elisabete Maria de Gouveia. Gas outflow in Seyfert galaxies: 3D radiative cooling hydrodynamical simulations. 2015, Anais.. Paris: International Astronomical Union, 2015. Disponível em: https://doi.org/10.1017/S1743921315002550. Acesso em: 07 out. 2024.

    • APA

      Melioli, C., & Dal Pino, E. M. de G. (2015). Gas outflow in Seyfert galaxies: 3D radiative cooling hydrodynamical simulations. In Proceedings IAU Symposium, 313: Extragalactic jets from every angle. Paris: International Astronomical Union. doi:10.1017/S1743921315002550

    • NLM

      Melioli C, Dal Pino EM de G. Gas outflow in Seyfert galaxies: 3D radiative cooling hydrodynamical simulations [Internet]. Proceedings IAU Symposium, 313: Extragalactic jets from every angle. 2015 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921315002550

    • Vancouver

      Melioli C, Dal Pino EM de G. Gas outflow in Seyfert galaxies: 3D radiative cooling hydrodynamical simulations [Internet]. Proceedings IAU Symposium, 313: Extragalactic jets from every angle. 2015 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921315002550

  • Trabalho de evento

    Bar effects on ionized gas properties and dust content in galaxy centers (2015)

    Zurita, A; Florido, E; Pérez, I; Coelho, Paula Rodrigues Teixeira; Gadotti, D. A

    Source: Galaxies in 3D across the Universe: Proceedings of the IAU Symposium, 309. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: GALÁXIAS ESPIRAIS, GALÁXIAS, GALÁXIAS, CENTRO GALÁCTICO

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      ZURITA, A et al. Bar effects on ionized gas properties and dust content in galaxy centers. 2015, Anais.. Paris: International Astronomical Union, 2015. Disponível em: https://doi.org/10.1017/S1743921314010473. Acesso em: 07 out. 2024.

    • APA

      Zurita, A., Florido, E., Pérez, I., Coelho, P. R. T., & Gadotti, D. A. (2015). Bar effects on ionized gas properties and dust content in galaxy centers. In Galaxies in 3D across the Universe: Proceedings of the IAU Symposium, 309. Paris: International Astronomical Union. doi:10.1017/S1743921314010473

    • NLM

      Zurita A, Florido E, Pérez I, Coelho PRT, Gadotti DA. Bar effects on ionized gas properties and dust content in galaxy centers [Internet]. Galaxies in 3D across the Universe: Proceedings of the IAU Symposium, 309. 2015 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921314010473

    • Vancouver

      Zurita A, Florido E, Pérez I, Coelho PRT, Gadotti DA. Bar effects on ionized gas properties and dust content in galaxy centers [Internet]. Galaxies in 3D across the Universe: Proceedings of the IAU Symposium, 309. 2015 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921314010473

  • Trabalho de evento

    3D studies of galaxies in compact groups (2015)

    Oliveira, Cláudia Lúcia Mendes de; Torres-Flores, Sérgio; Amram, Philippe; Plana, Henri; Epinat, Benoit

    Source: Galaxies in 3D across the Universe: Proceedings of the IAU Symposium, 309. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: GALÁXIAS ESPIRAIS, GALÁXIAS ELÍPTICAS, CINEMÁTICA, DINÂMICA DAS GALÁXIAS

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      OLIVEIRA, Cláudia Lúcia Mendes de et al. 3D studies of galaxies in compact groups. 2015, Anais.. Paris: International Astronomical Union, 2015. Disponível em: https://doi.org/10.1017/S1743921314009612. Acesso em: 07 out. 2024.

    • APA

      Oliveira, C. L. M. de, Torres-Flores, S., Amram, P., Plana, H., & Epinat, B. (2015). 3D studies of galaxies in compact groups. In Galaxies in 3D across the Universe: Proceedings of the IAU Symposium, 309. Paris: International Astronomical Union. doi:10.1017/S1743921314009612

    • NLM

      Oliveira CLM de, Torres-Flores S, Amram P, Plana H, Epinat B. 3D studies of galaxies in compact groups [Internet]. Galaxies in 3D across the Universe: Proceedings of the IAU Symposium, 309. 2015 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921314009612

    • Vancouver

      Oliveira CLM de, Torres-Flores S, Amram P, Plana H, Epinat B. 3D studies of galaxies in compact groups [Internet]. Galaxies in 3D across the Universe: Proceedings of the IAU Symposium, 309. 2015 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921314009612

  • Trabalho de evento

    Circumstellar polarimetry (2015)

    Magalhães, Antonio Mário; Carciofi, Alex Cavaliéri; Seriacopi, D. B

    Source: Polarimetry:from the Sun to Stars and Stellar Environments: Proceedings of IAU Symposium, 305. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: POLARIZAÇÃO (ASTRONOMIA), TRANSFERÊNCIA RADIATIVA, ATMOSFERAS ESTELARES

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      MAGALHÃES, Antonio Mário e CARCIOFI, Alex Cavaliéri e SERIACOPI, D. B. Circumstellar polarimetry. 2015, Anais.. Paris: International Astronomical Union, 2015. Disponível em: https://doi.org/10.1017/S1743921315004871. Acesso em: 07 out. 2024.

    • APA

      Magalhães, A. M., Carciofi, A. C., & Seriacopi, D. B. (2015). Circumstellar polarimetry. In Polarimetry:from the Sun to Stars and Stellar Environments: Proceedings of IAU Symposium, 305. Paris: International Astronomical Union. doi:10.1017/S1743921315004871

    • NLM

      Magalhães AM, Carciofi AC, Seriacopi DB. Circumstellar polarimetry [Internet]. Polarimetry:from the Sun to Stars and Stellar Environments: Proceedings of IAU Symposium, 305. 2015 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921315004871

    • Vancouver

      Magalhães AM, Carciofi AC, Seriacopi DB. Circumstellar polarimetry [Internet]. Polarimetry:from the Sun to Stars and Stellar Environments: Proceedings of IAU Symposium, 305. 2015 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921315004871

  • Trabalho de evento

    A 3D view of the Hydra I cluster core: II. Stellar populations (2015)

    Barbosa, Carlos Eduardo; Arnaboldi, Magda; Hilker, Michael; Coccato, Lodovico; Richtler,Tom; Oliveira, Cláudia Lúcia Mendes de

    Source: Galaxies in 3D across the Universe: Proceedings of the IAU Symposium, 309. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: GALÁXIAS ELÍPTICAS, POPULAÇÕES ESTELARES

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    • ABNT

      BARBOSA, Carlos Eduardo et al. A 3D view of the Hydra I cluster core: II. Stellar populations. 2015, Anais.. Paris: International Astronomical Union, 2015. Disponível em: https://doi.org/10.1017/S1743921314009727. Acesso em: 07 out. 2024.

    • APA

      Barbosa, C. E., Arnaboldi, M., Hilker, M., Coccato, L., Richtler, T., & Oliveira, C. L. M. de. (2015). A 3D view of the Hydra I cluster core: II. Stellar populations. In Galaxies in 3D across the Universe: Proceedings of the IAU Symposium, 309. Paris: International Astronomical Union. doi:10.1017/S1743921314009727

    • NLM

      Barbosa CE, Arnaboldi M, Hilker M, Coccato L, Richtler T, Oliveira CLM de. A 3D view of the Hydra I cluster core: II. Stellar populations [Internet]. Galaxies in 3D across the Universe: Proceedings of the IAU Symposium, 309. 2015 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921314009727

    • Vancouver

      Barbosa CE, Arnaboldi M, Hilker M, Coccato L, Richtler T, Oliveira CLM de. A 3D view of the Hydra I cluster core: II. Stellar populations [Internet]. Galaxies in 3D across the Universe: Proceedings of the IAU Symposium, 309. 2015 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921314009727

  • Trabalho de evento

    The circumstellar environment of the B[e] star GG Car: an interferometric modeling (2015)

    Souza, A. Domiciano de; Fernandes, M. Borges; Carciofi, Alex Cavaliéri; Chesneau, O

    Source: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of IAU Symposium, 307, 2014. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: ESTRELAS, INTERFEROMETRIA, ESPECTROSCOPIA, FOTOMETRIA

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      SOUZA, A. Domiciano de et al. The circumstellar environment of the B[e] star GG Car: an interferometric modeling. 2015, Anais.. Paris: International Astronomical Union, 2015. Disponível em: https://doi.org/10.1017/S1743921314006966. Acesso em: 07 out. 2024.

    • APA

      Souza, A. D. de, Fernandes, M. B., Carciofi, A. C., & Chesneau, O. (2015). The circumstellar environment of the B[e] star GG Car: an interferometric modeling. In New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of IAU Symposium, 307, 2014. Paris: International Astronomical Union. doi:10.1017/S1743921314006966

    • NLM

      Souza AD de, Fernandes MB, Carciofi AC, Chesneau O. The circumstellar environment of the B[e] star GG Car: an interferometric modeling [Internet]. New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of IAU Symposium, 307, 2014. 2015 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921314006966

    • Vancouver

      Souza AD de, Fernandes MB, Carciofi AC, Chesneau O. The circumstellar environment of the B[e] star GG Car: an interferometric modeling [Internet]. New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of IAU Symposium, 307, 2014. 2015 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921314006966

  • Trabalho de evento

    An empirical pipeline for determining the viscosity parameter for Be star disks (2015)

    Rímulo, Leandro R; Carciofi, Alex Cavaliéri; Rivinius, Thomas; Haubois, Xavier

    Source: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of IAU Symposium, 307. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: HIDRODINÂMICA, TRANSFERÊNCIA RADIATIVA, FOTOMETRIA, ESTRELAS, PERDA DE MASSA

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      RÍMULO, Leandro R et al. An empirical pipeline for determining the viscosity parameter for Be star disks. 2015, Anais.. Paris: International Astronomical Union, 2015. Disponível em: https://doi.org/10.1017/S1743921314006541. Acesso em: 07 out. 2024.

    • APA

      Rímulo, L. R., Carciofi, A. C., Rivinius, T., & Haubois, X. (2015). An empirical pipeline for determining the viscosity parameter for Be star disks. In New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of IAU Symposium, 307. Paris: International Astronomical Union. doi:10.1017/S1743921314006541

    • NLM

      Rímulo LR, Carciofi AC, Rivinius T, Haubois X. An empirical pipeline for determining the viscosity parameter for Be star disks [Internet]. New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of IAU Symposium, 307. 2015 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921314006541

    • Vancouver

      Rímulo LR, Carciofi AC, Rivinius T, Haubois X. An empirical pipeline for determining the viscosity parameter for Be star disks [Internet]. New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of IAU Symposium, 307. 2015 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921314006541

  • Trabalho de evento

    A 3D view of the Hydra I galaxy cluster core: I. Kinematic substructures (2015)

    Hilker, Michael; Barbosa, Carlos Eduardo; Richtler, Tom; Coccato, Lodovico; Arnaboldi, Magda; Oliveira, Cláudia Lúcia Mendes de

    Source: Galaxies in 3D across the Universe: Proceedings of the IAU Symposium, 309. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: GALÁXIAS ELÍPTICAS, DINÂMICA DAS GALÁXIAS, CINEMÁTICA

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      HILKER, Michael et al. A 3D view of the Hydra I galaxy cluster core: I. Kinematic substructures. 2015, Anais.. Paris: International Astronomical Union, 2015. Disponível em: https://doi.org/10.1017/S1743921314009715. Acesso em: 07 out. 2024.

    • APA

      Hilker, M., Barbosa, C. E., Richtler, T., Coccato, L., Arnaboldi, M., & Oliveira, C. L. M. de. (2015). A 3D view of the Hydra I galaxy cluster core: I. Kinematic substructures. In Galaxies in 3D across the Universe: Proceedings of the IAU Symposium, 309. Paris: International Astronomical Union. doi:10.1017/S1743921314009715

    • NLM

      Hilker M, Barbosa CE, Richtler T, Coccato L, Arnaboldi M, Oliveira CLM de. A 3D view of the Hydra I galaxy cluster core: I. Kinematic substructures [Internet]. Galaxies in 3D across the Universe: Proceedings of the IAU Symposium, 309. 2015 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921314009715

    • Vancouver

      Hilker M, Barbosa CE, Richtler T, Coccato L, Arnaboldi M, Oliveira CLM de. A 3D view of the Hydra I galaxy cluster core: I. Kinematic substructures [Internet]. Galaxies in 3D across the Universe: Proceedings of the IAU Symposium, 309. 2015 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921314009715

  • Trabalho de evento

    The photosphere and circumstellar environment of the Be star Achernar (2015)

    Faes, Daniel M; Souza, Armando Domiciano de; Carciofi, Alex Cavaliéri; Bendjoya, Philippe

    Source: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of the IAU Symposium, 307. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: ESTRELAS, INTERFEROMETRIA

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      FAES, Daniel M et al. The photosphere and circumstellar environment of the Be star Achernar. 2015, Anais.. Paris: International Astronomical Union, 2015. Disponível em: https://doi.org/10.1017/S1743921314006905. Acesso em: 07 out. 2024.

    • APA

      Faes, D. M., Souza, A. D. de, Carciofi, A. C., & Bendjoya, P. (2015). The photosphere and circumstellar environment of the Be star Achernar. In New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of the IAU Symposium, 307. Paris: International Astronomical Union. doi:10.1017/S1743921314006905

    • NLM

      Faes DM, Souza AD de, Carciofi AC, Bendjoya P. The photosphere and circumstellar environment of the Be star Achernar [Internet]. New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of the IAU Symposium, 307. 2015 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921314006905

    • Vancouver

      Faes DM, Souza AD de, Carciofi AC, Bendjoya P. The photosphere and circumstellar environment of the Be star Achernar [Internet]. New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of the IAU Symposium, 307. 2015 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921314006905

  • Trabalho de evento

    The Sun: a typical star in the solar neighborhood? (2014)

    Moreno, Jorge Luiz Meléndez

    Source: Setting the scene for Gaia and LAMOST: Proceedings IAU Symposium n. 298, 2013. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: SOL, ABUNDÂNCIAS SOLARES, ABUNDÂNCIA ESTELAR, FORMAÇÃO DO SISTEMA SOLAR, TERRA (PLANETA)

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      MORENO, Jorge Luiz Meléndez. The Sun: a typical star in the solar neighborhood? 2014, Anais.. Paris: International Astronomical Union, 2014. Disponível em: https://doi.org/10.1017/S1743921313006546. Acesso em: 07 out. 2024.

    • APA

      Moreno, J. L. M. (2014). The Sun: a typical star in the solar neighborhood? In Setting the scene for Gaia and LAMOST: Proceedings IAU Symposium n. 298, 2013. Paris: International Astronomical Union. doi:10.1017/S1743921313006546

    • NLM

      Moreno JLM. The Sun: a typical star in the solar neighborhood? [Internet]. Setting the scene for Gaia and LAMOST: Proceedings IAU Symposium n. 298, 2013. 2014 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921313006546

    • Vancouver

      Moreno JLM. The Sun: a typical star in the solar neighborhood? [Internet]. Setting the scene for Gaia and LAMOST: Proceedings IAU Symposium n. 298, 2013. 2014 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921313006546

  • Trabalho de evento

    Eliminating noise at the box-fitting spectrum (2014)

    Boufleur, Rodrigo Carlos; Emílio, Marcelo; Pacheco, Eduardo Janot; Reza, Jorge Ramiro de la; Rocha, José Carlos da

    Source: Formation, detection, and characterization of extrasolar habitable planets: Proceedings of IAU Symposium n. 293, 2012. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: FOTOMETRIA, ASTROFÍSICA

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      BOUFLEUR, Rodrigo Carlos et al. Eliminating noise at the box-fitting spectrum. 2014, Anais.. Paris: International Astronomical Union, 2014. Disponível em: https://doi.org/10.1017/S1743921313013288. Acesso em: 07 out. 2024.

    • APA

      Boufleur, R. C., Emílio, M., Pacheco, E. J., Reza, J. R. de la, & Rocha, J. C. da. (2014). Eliminating noise at the box-fitting spectrum. In Formation, detection, and characterization of extrasolar habitable planets: Proceedings of IAU Symposium n. 293, 2012. Paris: International Astronomical Union. doi:10.1017/S1743921313013288

    • NLM

      Boufleur RC, Emílio M, Pacheco EJ, Reza JR de la, Rocha JC da. Eliminating noise at the box-fitting spectrum [Internet]. Formation, detection, and characterization of extrasolar habitable planets: Proceedings of IAU Symposium n. 293, 2012. 2014 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921313013288

    • Vancouver

      Boufleur RC, Emílio M, Pacheco EJ, Reza JR de la, Rocha JC da. Eliminating noise at the box-fitting spectrum [Internet]. Formation, detection, and characterization of extrasolar habitable planets: Proceedings of IAU Symposium n. 293, 2012. 2014 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921313013288

  • Trabalho de evento

    Signatures of Earth-like planets in the chemical composition of solar-type stars (2014)

    Moreno, Jorge Luiz Meléndez; Ramírez, Iván

    Source: Formation, detection, and caracterization of extrasolar habitable planets: Proceedings of IAU Symposium n. 293, 2012. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: FORMAÇÃO DO SISTEMA SOLAR, TERRA (PLANETA), PLANETAS (SISTEMAS), ABUNDÂNCIA ESTELAR, FORMAÇÃO DE ESTRELAS

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      MORENO, Jorge Luiz Meléndez e RAMÍREZ, Iván. Signatures of Earth-like planets in the chemical composition of solar-type stars. 2014, Anais.. Paris: International Astronomical Union, 2014. Disponível em: https://doi.org/10.1017/S1743921313012519. Acesso em: 07 out. 2024.

    • APA

      Moreno, J. L. M., & Ramírez, I. (2014). Signatures of Earth-like planets in the chemical composition of solar-type stars. In Formation, detection, and caracterization of extrasolar habitable planets: Proceedings of IAU Symposium n. 293, 2012. Paris: International Astronomical Union. doi:10.1017/S1743921313012519

    • NLM

      Moreno JLM, Ramírez I. Signatures of Earth-like planets in the chemical composition of solar-type stars [Internet]. Formation, detection, and caracterization of extrasolar habitable planets: Proceedings of IAU Symposium n. 293, 2012. 2014 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921313012519

    • Vancouver

      Moreno JLM, Ramírez I. Signatures of Earth-like planets in the chemical composition of solar-type stars [Internet]. Formation, detection, and caracterization of extrasolar habitable planets: Proceedings of IAU Symposium n. 293, 2012. 2014 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921313012519

  • Trabalho de evento

    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

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      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: 07 out. 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 out. 07 ] 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 out. 07 ] Available from: https://doi.org/10.1017/S1743921311027694

  • Trabalho de evento

    Planetary nebulae and the chemical evolution of the galactic bulge: new abundances of older objects (2012)

    Cavichia, O; Costa, Roberto Dell'Aglio Dias da; Mollá, Mercedes; Maciel, Walter Junqueira

    Source: Proceedings of the International Astronomical Union: Planetary nebulae: an eye to the future. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: NEBULOSAS, GALÁXIAS, ABUNDÂNCIAS (ASTRONOMIA), FORMAÇÃO E EVOLUÇÃO DA GALÁXIA

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      CAVICHIA, O et al. Planetary nebulae and the chemical evolution of the galactic bulge: new abundances of older objects. 2012, Anais.. Paris: International Astronomical Union, 2012. Disponível em: https://doi.org/10.1017/S1743921312011258. Acesso em: 07 out. 2024.

    • APA

      Cavichia, O., Costa, R. D. 'A. D. da, Mollá, M., & Maciel, W. J. (2012). Planetary nebulae and the chemical evolution of the galactic bulge: new abundances of older objects. In Proceedings of the International Astronomical Union: Planetary nebulae: an eye to the future. Paris: International Astronomical Union. doi:10.1017/S1743921312011258

    • NLM

      Cavichia O, Costa RD'AD da, Mollá M, Maciel WJ. Planetary nebulae and the chemical evolution of the galactic bulge: new abundances of older objects [Internet]. Proceedings of the International Astronomical Union: Planetary nebulae: an eye to the future. 2012 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921312011258

    • Vancouver

      Cavichia O, Costa RD'AD da, Mollá M, Maciel WJ. Planetary nebulae and the chemical evolution of the galactic bulge: new abundances of older objects [Internet]. Proceedings of the International Astronomical Union: Planetary nebulae: an eye to the future. 2012 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921312011258

  • Trabalho de evento

    Radial abundance gradients from planetary nebulae and young objects: age effects (2012)

    Maciel, Walter Junqueira; Rodrigues, Thaise; Costa, Roberto Dell'Aglio Dias da

    Source: Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: ABUNDÂNCIAS (ASTRONOMIA), PLANETAS, GALÁXIA (VIA LÁCTEA)

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    • ABNT

      MACIEL, Walter Junqueira e RODRIGUES, Thaise e COSTA, Roberto Dell'Aglio Dias da. Radial abundance gradients from planetary nebulae and young objects: age effects. 2012, Anais.. Paris: International Astronomical Union, 2012. Disponível em: https://doi.org/10.1017/S174392131201174X. Acesso em: 07 out. 2024.

    • APA

      Maciel, W. J., Rodrigues, T., & Costa, R. D. 'A. D. da. (2012). Radial abundance gradients from planetary nebulae and young objects: age effects. In Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Paris: International Astronomical Union. doi:10.1017/S174392131201174X

    • NLM

      Maciel WJ, Rodrigues T, Costa RD'AD da. Radial abundance gradients from planetary nebulae and young objects: age effects [Internet]. Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. 2012 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S174392131201174X

    • Vancouver

      Maciel WJ, Rodrigues T, Costa RD'AD da. Radial abundance gradients from planetary nebulae and young objects: age effects [Internet]. Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. 2012 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S174392131201174X

  • Trabalho de evento

    Kinematic age determinations of planetary nebula central stars (2012)

    Rodrigues, Thaise S; Maciel, Walter Junqueira

    Source: Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: NEBULOSAS, PLANETAS, ESTRELAS

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    • ABNT

      RODRIGUES, Thaise S e MACIEL, Walter Junqueira. Kinematic age determinations of planetary nebula central stars. 2012, Anais.. Paris: International Astronomical Union, 2012. Disponível em: https://doi.org/10.1017/S1743921312012057. Acesso em: 07 out. 2024.

    • APA

      Rodrigues, T. S., & Maciel, W. J. (2012). Kinematic age determinations of planetary nebula central stars. In Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Paris: International Astronomical Union. doi:10.1017/S1743921312012057

    • NLM

      Rodrigues TS, Maciel WJ. Kinematic age determinations of planetary nebula central stars [Internet]. Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. 2012 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921312012057

    • Vancouver

      Rodrigues TS, Maciel WJ. Kinematic age determinations of planetary nebula central stars [Internet]. Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. 2012 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921312012057

  • Trabalho de evento

    Grids of synthetic spectra for H-poor central stars of planetary nebulae (CSPNe) (2012)

    Keller, Graziela R; Bianchi, Luciana; Herald, James E; Maciel, Walter Junqueira

    Source: Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Conference titles: IAU Symposium. Unidade: IAG

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

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    • ABNT

      KELLER, Graziela R et al. Grids of synthetic spectra for H-poor central stars of planetary nebulae (CSPNe). 2012, Anais.. Paris: International Astronomical Union, 2012. Disponível em: https://doi.org/10.1017/S1743921312011647. Acesso em: 07 out. 2024.

    • APA

      Keller, G. R., Bianchi, L., Herald, J. E., & Maciel, W. J. (2012). Grids of synthetic spectra for H-poor central stars of planetary nebulae (CSPNe). In Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Paris: International Astronomical Union. doi:10.1017/S1743921312011647

    • NLM

      Keller GR, Bianchi L, Herald JE, Maciel WJ. Grids of synthetic spectra for H-poor central stars of planetary nebulae (CSPNe) [Internet]. Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. 2012 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921312011647

    • Vancouver

      Keller GR, Bianchi L, Herald JE, Maciel WJ. Grids of synthetic spectra for H-poor central stars of planetary nebulae (CSPNe) [Internet]. Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. 2012 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921312011647

  • Trabalho de evento

    Physical parameters and chemical abundances in bipolar PNe (2012)

    Costa, Roberto Dell'Aglio Dias da; Faes, Daniel M; Morisset, Christophe

    Source: Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: ESPECTROSCOPIA, NEBULOSAS, ASTROQUÍMICA

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    • ABNT

      COSTA, Roberto Dell'Aglio Dias da e FAES, Daniel M e MORISSET, Christophe. Physical parameters and chemical abundances in bipolar PNe. 2012, Anais.. Paris: International Astronomical Union, 2012. Disponível em: https://doi.org/10.1017/S1743921312011301. Acesso em: 07 out. 2024.

    • APA

      Costa, R. D. 'A. D. da, Faes, D. M., & Morisset, C. (2012). Physical parameters and chemical abundances in bipolar PNe. In Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Paris: International Astronomical Union. doi:10.1017/S1743921312011301

    • NLM

      Costa RD'AD da, Faes DM, Morisset C. Physical parameters and chemical abundances in bipolar PNe [Internet]. Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. 2012 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921312011301

    • Vancouver

      Costa RD'AD da, Faes DM, Morisset C. Physical parameters and chemical abundances in bipolar PNe [Internet]. Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. 2012 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1017/S1743921312011301

  • Trabalho de evento

    Non-radial pulsations in the CoRoT Be Star 102761769 (2011)

    Janot Pacheco, Eduardo; Andrade, Laerte B. P. de; Emílio, Marcelo; Suárez, Juan Carlos; Jendreieck, Andressa

    Source: Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: ESTRELAS, ASTROFÍSICA ESTELAR

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    • ABNT

      JANOT PACHECO, Eduardo et al. Non-radial pulsations in the CoRoT Be Star 102761769. 2011, Anais.. Paris: International Astronomical Union, 2011. . Acesso em: 07 out. 2024.

    • APA

      Janot Pacheco, E., Andrade, L. B. P. de, Emílio, M., Suárez, J. C., & Jendreieck, A. (2011). Non-radial pulsations in the CoRoT Be Star 102761769. In Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Paris: International Astronomical Union.

    • NLM

      Janot Pacheco E, Andrade LBP de, Emílio M, Suárez JC, Jendreieck A. Non-radial pulsations in the CoRoT Be Star 102761769. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2024 out. 07 ]

    • Vancouver

      Janot Pacheco E, Andrade LBP de, Emílio M, Suárez JC, Jendreieck A. Non-radial pulsations in the CoRoT Be Star 102761769. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2024 out. 07 ]

  • Trabalho de evento-resumo

    Kenematic age determinations of planetary nebula central stars (2011)

    Rodrigues, T. S; Maciel, Walter Junqueira

    Source: Planetary nebulae: an eye to the future: Programme & abstracts. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: ESTRELAS, NEBULOSAS, PLANETAS, MEIO INTERESTELAR

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    • ABNT

      RODRIGUES, T. S e MACIEL, Walter Junqueira. Kenematic age determinations of planetary nebula central stars. 2011, Anais.. Paris: International Astronomical Union, 2011. . Acesso em: 07 out. 2024.

    • APA

      Rodrigues, T. S., & Maciel, W. J. (2011). Kenematic age determinations of planetary nebula central stars. In Planetary nebulae: an eye to the future: Programme & abstracts. Paris: International Astronomical Union.

    • NLM

      Rodrigues TS, Maciel WJ. Kenematic age determinations of planetary nebula central stars. Planetary nebulae: an eye to the future: Programme & abstracts. 2011 ;[citado 2024 out. 07 ]

    • Vancouver

      Rodrigues TS, Maciel WJ. Kenematic age determinations of planetary nebula central stars. Planetary nebulae: an eye to the future: Programme & abstracts. 2011 ;[citado 2024 out. 07 ]

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