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Trabalho de evento
The Sun: a typical star in the solar neighborhood? (2014)
Moreno, Jorge Luiz Meléndez
Fonte: Setting the scene for Gaia and LAMOST: Proceedings IAU Symposium n. 298, 2013. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: 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: 14 out. 2025.
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 2025 out. 14 ] 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 2025 out. 14 ] 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
Fonte: Formation, detection, and characterization of extrasolar habitable planets: Proceedings of IAU Symposium n. 293, 2012. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: 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: 14 out. 2025.
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 2025 out. 14 ] 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 2025 out. 14 ] 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
Fonte: Formation, detection, and caracterization of extrasolar habitable planets: Proceedings of IAU Symposium n. 293, 2012. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: 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: 14 out. 2025.
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 2025 out. 14 ] 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 2025 out. 14 ] Available from: https://doi.org/10.1017/S1743921313012519
Trabalho de evento
Planetary nebulae and determination of the bulge–disk boundary (2013)
Costa, Roberto Dell'Aglio Dias da; Cavichia, Oscar; Maciel, Walter Junqueira
Fonte: Advancing the Physics of Cosmic Distances: Proceedings of IAU Symposium n. 289, 2012. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESPECTROSCOPIA, NEBULOSAS, PLANETAS, ESTRUTURA DA GALÁXIA
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COSTA, Roberto Dell'Aglio Dias da e CAVICHIA, Oscar e MACIEL, Walter Junqueira. Planetary nebulae and determination of the bulge–disk boundary. 2013, Anais.. Paris: International Astronomical Union, 2013. Disponível em: https://doi.org/10.1017/S1743921312021746. Acesso em: 14 out. 2025.
APA
Costa, R. D. 'A. D. da, Cavichia, O., & Maciel, W. J. (2013). Planetary nebulae and determination of the bulge–disk boundary. In Advancing the Physics of Cosmic Distances: Proceedings of IAU Symposium n. 289, 2012. Paris: International Astronomical Union. doi:10.1017/S1743921312021746
NLM
Costa RD'AD da, Cavichia O, Maciel WJ. Planetary nebulae and determination of the bulge–disk boundary [Internet]. Advancing the Physics of Cosmic Distances: Proceedings of IAU Symposium n. 289, 2012. 2013 ;[citado 2025 out. 14 ] Available from: https://doi.org/10.1017/S1743921312021746
Vancouver
Costa RD'AD da, Cavichia O, Maciel WJ. Planetary nebulae and determination of the bulge–disk boundary [Internet]. Advancing the Physics of Cosmic Distances: Proceedings of IAU Symposium n. 289, 2012. 2013 ;[citado 2025 out. 14 ] Available from: https://doi.org/10.1017/S1743921312021746
Trabalho de evento
Turbulence and dynamo interlinks (2013)
Dal Pino, Elisabete Maria de Gouveia; Santos-Lima, R; Kowal, G; Falceta-Gonçalves, D
Fonte: Solar and Astrophysical Dynamos and Magnetic Activity: Proceedings of IAU Symposium n. 294, 2012. Nome do evento: IAU Symposium. Unidades: IAG, EACH
Assuntos: MAGNETOHIDRODINÂMICA, TURBULÊNCIA, DÍNAMOS, MAGNETISMO, MEIO INTERGALÁTICO
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DAL PINO, Elisabete Maria de Gouveia et al. Turbulence and dynamo interlinks. 2013, Anais.. Paris: International Astronomical Union, 2013. Disponível em: https://doi.org/10.1017/S174392131300272X. Acesso em: 14 out. 2025.
APA
Dal Pino, E. M. de G., Santos-Lima, R., Kowal, G., & Falceta-Gonçalves, D. (2013). Turbulence and dynamo interlinks. In Solar and Astrophysical Dynamos and Magnetic Activity: Proceedings of IAU Symposium n. 294, 2012. Paris: International Astronomical Union. doi:10.1017/S174392131300272X
NLM
Dal Pino EM de G, Santos-Lima R, Kowal G, Falceta-Gonçalves D. Turbulence and dynamo interlinks [Internet]. Solar and Astrophysical Dynamos and Magnetic Activity: Proceedings of IAU Symposium n. 294, 2012. 2013 ;[citado 2025 out. 14 ] Available from: https://doi.org/10.1017/S174392131300272X
Vancouver
Dal Pino EM de G, Santos-Lima R, Kowal G, Falceta-Gonçalves D. Turbulence and dynamo interlinks [Internet]. Solar and Astrophysical Dynamos and Magnetic Activity: Proceedings of IAU Symposium n. 294, 2012. 2013 ;[citado 2025 out. 14 ] Available from: https://doi.org/10.1017/S174392131300272X
Trabalho de evento
Prospect on intergalactic magnetic field measurements with gamma-ray instruments (2013)
Sol, Helène; Zech, Andreas; Boisson, Catherine; Krawczynski, Henric; Fallon, Lisa; Dal Pino, Elisabete Maria de Gouveia; Hinton, Jim; Inoue, Susumu; Neronov, Andrii; White, Richard
Fonte: Solar and Astrophysical Dynamos and Magnetic Activity: Proceedings of IAU Symposium n. 294, 2012. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: CAMPO MAGNÉTICO, RAIOS GAMA, GALÁXIAS, MEIO INTERGALÁTICO
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ABNT
SOL, Helène et al. Prospect on intergalactic magnetic field measurements with gamma-ray instruments. 2013, Anais.. Paris: International Astronomical Union, 2013. Disponível em: https://doi.org/10.1017/S1743921313002925. Acesso em: 14 out. 2025.
APA
Sol, H., Zech, A., Boisson, C., Krawczynski, H., Fallon, L., Dal Pino, E. M. de G., et al. (2013). Prospect on intergalactic magnetic field measurements with gamma-ray instruments. In Solar and Astrophysical Dynamos and Magnetic Activity: Proceedings of IAU Symposium n. 294, 2012. Paris: International Astronomical Union. doi:10.1017/S1743921313002925
NLM
Sol H, Zech A, Boisson C, Krawczynski H, Fallon L, Dal Pino EM de G, Hinton J, Inoue S, Neronov A, White R. Prospect on intergalactic magnetic field measurements with gamma-ray instruments [Internet]. Solar and Astrophysical Dynamos and Magnetic Activity: Proceedings of IAU Symposium n. 294, 2012. 2013 ;[citado 2025 out. 14 ] Available from: https://doi.org/10.1017/S1743921313002925
Vancouver
Sol H, Zech A, Boisson C, Krawczynski H, Fallon L, Dal Pino EM de G, Hinton J, Inoue S, Neronov A, White R. Prospect on intergalactic magnetic field measurements with gamma-ray instruments [Internet]. Solar and Astrophysical Dynamos and Magnetic Activity: Proceedings of IAU Symposium n. 294, 2012. 2013 ;[citado 2025 out. 14 ] Available from: https://doi.org/10.1017/S1743921313002925
Trabalho de evento
Magnetic color-flavor-locked stars (2013)
Paulucci, Laura; Ferrer, Efrain J; Incera, Vivian de la; Horvath, Jorge Ernesto
Fonte: Neutron Stars and Pulsars: Challenges and Opportunities after 80 Years: Proceedings. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESTRELAS DE NEUTRONS, CAMPO MAGNÉTICO, ESTRELAS
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PAULUCCI, Laura et al. Magnetic color-flavor-locked stars. 2013, Anais.. Paris: International Astronomical Union, 2013. Disponível em: https://doi.org/10.1017/S1743921312024532. Acesso em: 14 out. 2025.
APA
Paulucci, L., Ferrer, E. J., Incera, V. de la, & Horvath, J. E. (2013). Magnetic color-flavor-locked stars. In Neutron Stars and Pulsars: Challenges and Opportunities after 80 Years: Proceedings. Paris: International Astronomical Union. doi:10.1017/S1743921312024532
NLM
Paulucci L, Ferrer EJ, Incera V de la, Horvath JE. Magnetic color-flavor-locked stars [Internet]. Neutron Stars and Pulsars: Challenges and Opportunities after 80 Years: Proceedings. 2013 ;[citado 2025 out. 14 ] Available from: https://doi.org/10.1017/S1743921312024532
Vancouver
Paulucci L, Ferrer EJ, Incera V de la, Horvath JE. Magnetic color-flavor-locked stars [Internet]. Neutron Stars and Pulsars: Challenges and Opportunities after 80 Years: Proceedings. 2013 ;[citado 2025 out. 14 ] Available from: https://doi.org/10.1017/S1743921312024532
Trabalho de evento
The star formation rate in the inner Milky Way Galaxy (2013)
Cavichia, Oscar; Mollá, Mercedes; Costa, Roberto Dell'Aglio Dias da; Maciel, Walter Junqueira
Fonte: Molecular Gas, Dust, and Star Formation in Galaxies: Proceedings of IAU Symposium n. 292, 2012. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIAS (ASTRONOMIA), FORMAÇÃO E EVOLUÇÃO DA GALÁXIA
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CAVICHIA, Oscar et al. The star formation rate in the inner Milky Way Galaxy. 2013, Anais.. Paris: International Astronomical Union, 2013. Disponível em: https://doi.org/10.1017/S1743921313000586. Acesso em: 14 out. 2025.
APA
Cavichia, O., Mollá, M., Costa, R. D. 'A. D. da, & Maciel, W. J. (2013). The star formation rate in the inner Milky Way Galaxy. In Molecular Gas, Dust, and Star Formation in Galaxies: Proceedings of IAU Symposium n. 292, 2012. Paris: International Astronomical Union. doi:10.1017/S1743921313000586
NLM
Cavichia O, Mollá M, Costa RD'AD da, Maciel WJ. The star formation rate in the inner Milky Way Galaxy [Internet]. Molecular Gas, Dust, and Star Formation in Galaxies: Proceedings of IAU Symposium n. 292, 2012. 2013 ;[citado 2025 out. 14 ] Available from: https://doi.org/10.1017/S1743921313000586
Vancouver
Cavichia O, Mollá M, Costa RD'AD da, Maciel WJ. The star formation rate in the inner Milky Way Galaxy [Internet]. Molecular Gas, Dust, and Star Formation in Galaxies: Proceedings of IAU Symposium n. 292, 2012. 2013 ;[citado 2025 out. 14 ] Available from: https://doi.org/10.1017/S1743921313000586
Trabalho de evento
Bimodal chemical evolution of the Galactic disk and the Barium abundance of Cepheids (2013)
Lépine, Jacques Raymond Daniel; Andrievky, Sergei; Barros, Douglas; Junqueira, Thiago C; Scarano Jr., Sergio
Fonte: Setting the scene for Gaia and LAMOST: Proceedings of IAU Symposium n. 298, 2013. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: GALÁXIA (VIA LÁCTEA), GALÁXIAS ESPIRAIS, ESTRELAS, ABUNDÂNCIAS (ASTRONOMIA), FORMAÇÃO E EVOLUÇÃO DA GALÁXIA
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LÉPINE, Jacques Raymond Daniel et al. Bimodal chemical evolution of the Galactic disk and the Barium abundance of Cepheids. 2013, Anais.. Paris: International Astronomical Union, 2013. Disponível em: https://doi.org/10.1017/S174392131300625X. Acesso em: 14 out. 2025.
APA
Lépine, J. R. D., Andrievky, S., Barros, D., Junqueira, T. C., & Scarano Jr., S. (2013). Bimodal chemical evolution of the Galactic disk and the Barium abundance of Cepheids. In Setting the scene for Gaia and LAMOST: Proceedings of IAU Symposium n. 298, 2013. Paris: International Astronomical Union. doi:10.1017/S174392131300625X
NLM
Lépine JRD, Andrievky S, Barros D, Junqueira TC, Scarano Jr. S. Bimodal chemical evolution of the Galactic disk and the Barium abundance of Cepheids [Internet]. Setting the scene for Gaia and LAMOST: Proceedings of IAU Symposium n. 298, 2013. 2013 ;[citado 2025 out. 14 ] Available from: https://doi.org/10.1017/S174392131300625X
Vancouver
Lépine JRD, Andrievky S, Barros D, Junqueira TC, Scarano Jr. S. Bimodal chemical evolution of the Galactic disk and the Barium abundance of Cepheids [Internet]. Setting the scene for Gaia and LAMOST: Proceedings of IAU Symposium n. 298, 2013. 2013 ;[citado 2025 out. 14 ] Available from: https://doi.org/10.1017/S174392131300625X
Trabalho de evento
Trigonometric parallaxes in the TW Hydrae Association (2013)
Ducourant, C; Teixeira, Ramachrisna; Chauvin, G; Krone-Martins, A; Le Campion, J. F; Galli, P; Song, I; Zuckerman, B.
Fonte: Advancing the Physics of Cosmic Distances: Proceedings of IAU Symposium n. 289,2012. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ASTROMETRIA, DISTÂNCIAS ESTELARES, CINEMÁTICA, EVOLUÇÃO ESTELAR
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DUCOURANT, C et al. Trigonometric parallaxes in the TW Hydrae Association. 2013, Anais.. Paris: International Astronomical Union, 2013. Disponível em: https://doi.org/10.1017/S1743921312021771. Acesso em: 14 out. 2025.
APA
Ducourant, C., Teixeira, R., Chauvin, G., Krone-Martins, A., Le Campion, J. F., Galli, P., et al. (2013). Trigonometric parallaxes in the TW Hydrae Association. In Advancing the Physics of Cosmic Distances: Proceedings of IAU Symposium n. 289,2012. Paris: International Astronomical Union. doi:10.1017/S1743921312021771
NLM
Ducourant C, Teixeira R, Chauvin G, Krone-Martins A, Le Campion JF, Galli P, Song I, Zuckerman B. Trigonometric parallaxes in the TW Hydrae Association [Internet]. Advancing the Physics of Cosmic Distances: Proceedings of IAU Symposium n. 289,2012. 2013 ;[citado 2025 out. 14 ] Available from: https://doi.org/10.1017/S1743921312021771
Vancouver
Ducourant C, Teixeira R, Chauvin G, Krone-Martins A, Le Campion JF, Galli P, Song I, Zuckerman B. Trigonometric parallaxes in the TW Hydrae Association [Internet]. Advancing the Physics of Cosmic Distances: Proceedings of IAU Symposium n. 289,2012. 2013 ;[citado 2025 out. 14 ] Available from: https://doi.org/10.1017/S1743921312021771
Trabalho de evento
Kinematic distances of pre-main-sequence stars in the Lupus star-forming region (2013)
Galli, P. A. B; Teixeira, Ramachrisna; Ducourant, C; Bertout, C
Fonte: Advancing the Physics of Cosmic Distances: Proceedings of IAU Symposium n. 289, 2012. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESTRELAS, DISTÂNCIAS ESTELARES, MEIO INTERESTELAR
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ABNT
GALLI, P. A. B et al. Kinematic distances of pre-main-sequence stars in the Lupus star-forming region. 2013, Anais.. Paris: International Astronomical Union, 2013. Disponível em: https://doi.org/10.1017/S1743921312021783. Acesso em: 14 out. 2025.
APA
Galli, P. A. B., Teixeira, R., Ducourant, C., & Bertout, C. (2013). Kinematic distances of pre-main-sequence stars in the Lupus star-forming region. In Advancing the Physics of Cosmic Distances: Proceedings of IAU Symposium n. 289, 2012. Paris: International Astronomical Union. doi:10.1017/S1743921312021783
NLM
Galli PAB, Teixeira R, Ducourant C, Bertout C. Kinematic distances of pre-main-sequence stars in the Lupus star-forming region [Internet]. Advancing the Physics of Cosmic Distances: Proceedings of IAU Symposium n. 289, 2012. 2013 ;[citado 2025 out. 14 ] Available from: https://doi.org/10.1017/S1743921312021783
Vancouver
Galli PAB, Teixeira R, Ducourant C, Bertout C. Kinematic distances of pre-main-sequence stars in the Lupus star-forming region [Internet]. Advancing the Physics of Cosmic Distances: Proceedings of IAU Symposium n. 289, 2012. 2013 ;[citado 2025 out. 14 ] Available from: https://doi.org/10.1017/S1743921312021783
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
Fonte: Proceedings of the International Astronomical Union: From Interacting Binaries to Exoplanets: Essential Modeling Tools. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESTRELAS BINÁRIAS, PERDA DE MASSA, VENTO, ESTRELAS
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ABNT
MENNICKENT, Ronald E et al. Optical spectroscopy of V393 Scorpii during its long cycle. 2012, Anais.. Paris: International Astronomical Union, 2012. Disponível em: https://doi.org/10.1017/S1743921311027694. Acesso em: 14 out. 2025.
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 2025 out. 14 ] 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 2025 out. 14 ] 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
Fonte: Proceedings of the International Astronomical Union: Planetary nebulae: an eye to the future. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: NEBULOSAS, GALÁXIAS, ABUNDÂNCIAS (ASTRONOMIA), FORMAÇÃO E EVOLUÇÃO DA GALÁXIA
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ABNT
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: 14 out. 2025.
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 2025 out. 14 ] 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 2025 out. 14 ] 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
Fonte: Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: 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: 14 out. 2025.
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 2025 out. 14 ] 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 2025 out. 14 ] 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
Fonte: Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: 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: 14 out. 2025.
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 2025 out. 14 ] 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 2025 out. 14 ] 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
Fonte: Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESTRELAS, ATMOSFERAS ESTELARES, PERDA DE MASSA, VENTO
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 14 out. 2025.
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 2025 out. 14 ] 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 2025 out. 14 ] 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
Fonte: Planetary nebulae: an eye to the future: Proceedings IAU Symposium n. 283, 2011. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESPECTROSCOPIA, NEBULOSAS, ASTROQUÍMICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 14 out. 2025.
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 2025 out. 14 ] 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 2025 out. 14 ] 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
Fonte: Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESTRELAS, ASTROFÍSICA ESTELAR
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
JANOT PACHECO, Eduardo et al. Non-radial pulsations in the CoRoT Be Star 102761769. 2011, Anais.. Paris: International Astronomical Union, 2011. . Acesso em: 14 out. 2025.
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 2025 out. 14 ]
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 2025 out. 14 ]
Trabalho de evento-resumo
Kenematic age determinations of planetary nebula central stars (2011)
Rodrigues, T. S; Maciel, Walter Junqueira
Fonte: Planetary nebulae: an eye to the future: Programme & abstracts. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESTRELAS, NEBULOSAS, PLANETAS, MEIO INTERESTELAR
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 14 out. 2025.
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 2025 out. 14 ]
Vancouver
Rodrigues TS, Maciel WJ. Kenematic age determinations of planetary nebula central stars. Planetary nebulae: an eye to the future: Programme & abstracts. 2011 ;[citado 2025 out. 14 ]
Trabalho de evento
Discussion: Normal and active OB stars as extreme condition test beds (2011)
Gagné, Marc; Janot-Pacheco, Eduardo
Fonte: Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESTRELAS, ASTROFÍSICA ESTELAR
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
GAGNÉ, Marc e JANOT-PACHECO, Eduardo. Discussion: Normal and active OB stars as extreme condition test beds. 2011, Anais.. Paris: International Astronomical Union, 2011. Disponível em: https://doi.org/10.1017/S1743921311011483. Acesso em: 14 out. 2025.
APA
Gagné, M., & Janot-Pacheco, E. (2011). Discussion: Normal and active OB stars as extreme condition test beds. In Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Paris: International Astronomical Union. doi:10.1017/S1743921311011483
NLM
Gagné M, Janot-Pacheco E. Discussion: Normal and active OB stars as extreme condition test beds [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2025 out. 14 ] Available from: https://doi.org/10.1017/S1743921311011483
Vancouver
Gagné M, Janot-Pacheco E. Discussion: Normal and active OB stars as extreme condition test beds [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2025 out. 14 ] Available from: https://doi.org/10.1017/S1743921311011483

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