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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
Fonte: Proceedings IAU Symposium, 313: Extragalactic jets from every angle. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: GALÁXIAS SEY FERT, JATOS (ASTRONOMIA), HIDRODINÂMICA
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ABNT
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
Fonte: Galaxies in 3D across the Universe: Proceedings of the IAU Symposium, 309. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: 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
Circumstellar polarimetry (2015)
Magalhães, Antonio Mário; Carciofi, Alex Cavaliéri; Seriacopi, D. B
Fonte: Polarimetry:from the Sun to Stars and Stellar Environments: Proceedings of IAU Symposium, 305. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: 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
Fonte: Galaxies in 3D across the Universe: Proceedings of the IAU Symposium, 309. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: GALÁXIAS ELÍPTICAS, POPULAÇÕES ESTELARES
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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
Fonte: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of IAU Symposium, 307, 2014. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESTRELAS, INTERFEROMETRIA, ESPECTROSCOPIA, FOTOMETRIA
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ABNT
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
Fonte: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of IAU Symposium, 307. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: 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
Fonte: Galaxies in 3D across the Universe: Proceedings of the IAU Symposium, 309. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: GALÁXIAS ELÍPTICAS, DINÂMICA DAS GALÁXIAS, CINEMÁTICA
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ABNT
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
Fonte: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of the IAU Symposium, 307. Nome do evento: IAU Symposium. Unidade: IAG
Assuntos: ESTRELAS, INTERFEROMETRIA
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ABNT
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
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: 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
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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ABNT
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
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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ABNT
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
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: 07 out. 2024.
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 2024 out. 07 ] 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 2024 out. 07 ] 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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ABNT
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: 07 out. 2024.
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 2024 out. 07 ] 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 2024 out. 07 ] 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: 07 out. 2024.
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 2024 out. 07 ] 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 2024 out. 07 ] 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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ABNT
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: 07 out. 2024.
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 2024 out. 07 ] 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 2024 out. 07 ] 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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
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: 07 out. 2024.
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 2024 out. 07 ] 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 2024 out. 07 ] 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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
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: 07 out. 2024.
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 2024 out. 07 ] 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 2024 out. 07 ] 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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
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: 07 out. 2024.
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 2024 out. 07 ] 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 2024 out. 07 ] 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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 07 out. 2024.
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 2024 out. 07 ] 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 2024 out. 07 ] 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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 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

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