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  • Fonte: Astrophysical Journal. Unidade: IAG

    Assunto: ESTRELAS BINÁRIAS

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      MARR, K. C et al. The role of disk tearing and precession in the observed variability of pleione. Astrophysical Journal, v. 928, p. 145, 2022Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ac4266. Acesso em: 21 jul. 2024.
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      Marr, K. C., Jones, C. E., Tycner, C., Carciofi, A. C., & Silva, F. A. C. (2022). The role of disk tearing and precession in the observed variability of pleione. Astrophysical Journal, 928, 145. doi:10.3847/1538-4357/ac4266
    • NLM

      Marr KC, Jones CE, Tycner C, Carciofi AC, Silva FAC. The role of disk tearing and precession in the observed variability of pleione [Internet]. Astrophysical Journal. 2022 ;928 145.[citado 2024 jul. 21 ] Available from: https://doi.org/10.3847/1538-4357/ac4266
    • Vancouver

      Marr KC, Jones CE, Tycner C, Carciofi AC, Silva FAC. The role of disk tearing and precession in the observed variability of pleione [Internet]. Astrophysical Journal. 2022 ;928 145.[citado 2024 jul. 21 ] Available from: https://doi.org/10.3847/1538-4357/ac4266
  • Fonte: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Assuntos: ATMOSFERAS ESTELARES, ABUNDÂNCIA ESTELAR, ESTRELAS

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      ERNANDES, H et al. Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy. Monthly Notices of the Royal Astronomical Society, v. 510, p. 5362-5375, 2022Tradução . . Disponível em: https://doi.org/10.1093/mnras/stab3789. Acesso em: 21 jul. 2024.
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      Ernandes, H., Barbuy, B. L. S., Friaça, A. C. S., Hill, V., Spite, M., Spite, F., et al. (2022). Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy. Monthly Notices of the Royal Astronomical Society, 510, 5362-5375. doi:10.1093/mnras/stab3789
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      Ernandes H, Barbuy BLS, Friaça ACS, Hill V, Spite M, Spite F, Castilho BV, Evans CJ. Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 510 5362-5375.[citado 2024 jul. 21 ] Available from: https://doi.org/10.1093/mnras/stab3789
    • Vancouver

      Ernandes H, Barbuy BLS, Friaça ACS, Hill V, Spite M, Spite F, Castilho BV, Evans CJ. Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 510 5362-5375.[citado 2024 jul. 21 ] Available from: https://doi.org/10.1093/mnras/stab3789
  • Fonte: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Assuntos: COSMOLOGIA, AGLOMERADOS DE GALÁXIAS, UNIVERSO PRIMORDIAL, FOTOMETRIA

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      GONÇALVES, Geraldo et al. How well can we determine ages and chemical abundances from spectral fitting of integrated light spectra?. Monthly Notices of the Royal Astronomical Society, v. 499, n. 2, p. 2327–2339, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/staa3051. Acesso em: 21 jul. 2024.
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      Gonçalves, G., Coelho, P., Shiavon, R., & Usher, C. (2020). How well can we determine ages and chemical abundances from spectral fitting of integrated light spectra? Monthly Notices of the Royal Astronomical Society, 499( 2), 2327–2339. doi:10.1093/mnras/staa3051
    • NLM

      Gonçalves G, Coelho P, Shiavon R, Usher C. How well can we determine ages and chemical abundances from spectral fitting of integrated light spectra? [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 499( 2): 2327–2339.[citado 2024 jul. 21 ] Available from: https://doi.org/10.1093/mnras/staa3051
    • Vancouver

      Gonçalves G, Coelho P, Shiavon R, Usher C. How well can we determine ages and chemical abundances from spectral fitting of integrated light spectra? [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 499( 2): 2327–2339.[citado 2024 jul. 21 ] Available from: https://doi.org/10.1093/mnras/staa3051
  • Fonte: Astronomy and Astrophysics. Unidade: IAG

    Assuntos: ESPECTROS, GALÁXIAS

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      GONNEAU, A e LYUBENOVA, M e COELHO, Paula Rodrigues Teixeira. The X-shooter spectral library (xsl): data release 2?,??. Astronomy and Astrophysics, v. 634, p. A133, 2020Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201936825. Acesso em: 21 jul. 2024.
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      Gonneau, A., Lyubenova, M., & Coelho, P. R. T. (2020). The X-shooter spectral library (xsl): data release 2?,?? Astronomy and Astrophysics, 634, A133. doi:10.1051/0004-6361/201936825
    • NLM

      Gonneau A, Lyubenova M, Coelho PRT. The X-shooter spectral library (xsl): data release 2?,?? [Internet]. Astronomy and Astrophysics. 2020 ; 634 A133.[citado 2024 jul. 21 ] Available from: https://doi.org/10.1051/0004-6361/201936825
    • Vancouver

      Gonneau A, Lyubenova M, Coelho PRT. The X-shooter spectral library (xsl): data release 2?,?? [Internet]. Astronomy and Astrophysics. 2020 ; 634 A133.[citado 2024 jul. 21 ] Available from: https://doi.org/10.1051/0004-6361/201936825
  • Fonte: Astrophysical Journal. Unidade: IAG

    Assuntos: TRANSFERÊNCIA RADIATIVA, ESTRELAS BINÁRIAS

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      SUFFAK, M W et al. The Large-scale Behavior in the Disk of δ Scorpii from 2000 to 2018. Astrophysical Journal, v. 890, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab68dc. Acesso em: 21 jul. 2024.
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      Suffak, M. W., Richardson, N. D., Jones, C. E., Tycner, C., Henry, G. W., Carciofi, A. C., et al. (2020). The Large-scale Behavior in the Disk of δ Scorpii from 2000 to 2018. Astrophysical Journal, 890. doi:10.3847/1538-4357/ab68dc
    • NLM

      Suffak MW, Richardson ND, Jones CE, Tycner C, Henry GW, Carciofi AC, Mota BC, Rubio AC. The Large-scale Behavior in the Disk of δ Scorpii from 2000 to 2018 [Internet]. Astrophysical Journal. 2020 ;890[citado 2024 jul. 21 ] Available from: https://doi.org/10.3847/1538-4357/ab68dc
    • Vancouver

      Suffak MW, Richardson ND, Jones CE, Tycner C, Henry GW, Carciofi AC, Mota BC, Rubio AC. The Large-scale Behavior in the Disk of δ Scorpii from 2000 to 2018 [Internet]. Astrophysical Journal. 2020 ;890[citado 2024 jul. 21 ] Available from: https://doi.org/10.3847/1538-4357/ab68dc
  • Fonte: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Assuntos: GALÁXIAS, ESPECTROSCOPIA, PROCESSAMENTO DE IMAGENS

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      GONZALEZ-GAITAN, S et al. Spatial field reconstruction with INLA: application to IFU galaxy data. Monthly Notices of the Royal Astronomical Society, v. 482, n. 3, p. 3880-3891, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty2881. Acesso em: 21 jul. 2024.
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      Gonzalez-Gaitan, S., Souza, R. S. de, Krone-Martins, A., Cameron, E., Coelho, P. R. T., Galbany, L., & Ishida, E. E. O. (2019). Spatial field reconstruction with INLA: application to IFU galaxy data. Monthly Notices of the Royal Astronomical Society, 482( 3), 3880-3891. doi:10.1093/mnras/sty2881
    • NLM

      Gonzalez-Gaitan S, Souza RS de, Krone-Martins A, Cameron E, Coelho PRT, Galbany L, Ishida EEO. Spatial field reconstruction with INLA: application to IFU galaxy data [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 482( 3): 3880-3891.[citado 2024 jul. 21 ] Available from: https://doi.org/10.1093/mnras/sty2881
    • Vancouver

      Gonzalez-Gaitan S, Souza RS de, Krone-Martins A, Cameron E, Coelho PRT, Galbany L, Ishida EEO. Spatial field reconstruction with INLA: application to IFU galaxy data [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 482( 3): 3880-3891.[citado 2024 jul. 21 ] Available from: https://doi.org/10.1093/mnras/sty2881
  • Fonte: The Astrophysical Journal. Unidade: IAG

    Assuntos: CAMPO MAGNÉTICO, ASTROFÍSICA SOLAR

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      GUERRERO, G et al. What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars?. The Astrophysical Journal, v. 880, n. 1, p. 6/1-6/20, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab224a. Acesso em: 21 jul. 2024.
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      Guerrero, G., Zaire, B., Smolarkiewicz, P. K., Dal Pino, E. M. de G., Kosovichev, A. G., & Mansour, N. N. (2019). What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars? The Astrophysical Journal, 880( 1), 6/1-6/20. doi:10.3847/1538-4357/ab224a
    • NLM

      Guerrero G, Zaire B, Smolarkiewicz PK, Dal Pino EM de G, Kosovichev AG, Mansour NN. What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars? [Internet]. The Astrophysical Journal. 2019 ; 880( 1): 6/1-6/20.[citado 2024 jul. 21 ] Available from: https://doi.org/10.3847/1538-4357/ab224a
    • Vancouver

      Guerrero G, Zaire B, Smolarkiewicz PK, Dal Pino EM de G, Kosovichev AG, Mansour NN. What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars? [Internet]. The Astrophysical Journal. 2019 ; 880( 1): 6/1-6/20.[citado 2024 jul. 21 ] Available from: https://doi.org/10.3847/1538-4357/ab224a
  • Fonte: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Assuntos: MEIO INTERESTELAR, NEBULOSAS

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      ALEMAN, Isabel et al. Herschel Planetary Nebula Survey (HerPlaNS)★: hydrogen recombination laser lines in Mz 3. Monthly Notices of the Royal Astronomical Society, v. 475, p. 4499-4510, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty966. Acesso em: 21 jul. 2024.
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      Aleman, I., Exter, K., Ueta, T., Walton, S., Tielens, A. G. G. M., Zijlstra, A., et al. (2018). Herschel Planetary Nebula Survey (HerPlaNS)★: hydrogen recombination laser lines in Mz 3. Monthly Notices of the Royal Astronomical Society, 475, 4499-4510. doi:10.1093/mnras/sty966
    • NLM

      Aleman I, Exter K, Ueta T, Walton S, Tielens AGGM, Zijlstra A, Montez Jr. R, Abraham Z, Otsuka M, Beaklini PPB, Van Hoof PAM, Villaver E, Leal-Ferreira ML, Mendonza E, Lépine JRD. Herschel Planetary Nebula Survey (HerPlaNS)★: hydrogen recombination laser lines in Mz 3 [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ;475 4499-4510.[citado 2024 jul. 21 ] Available from: https://doi.org/10.1093/mnras/sty966
    • Vancouver

      Aleman I, Exter K, Ueta T, Walton S, Tielens AGGM, Zijlstra A, Montez Jr. R, Abraham Z, Otsuka M, Beaklini PPB, Van Hoof PAM, Villaver E, Leal-Ferreira ML, Mendonza E, Lépine JRD. Herschel Planetary Nebula Survey (HerPlaNS)★: hydrogen recombination laser lines in Mz 3 [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ;475 4499-4510.[citado 2024 jul. 21 ] Available from: https://doi.org/10.1093/mnras/sty966
  • Fonte: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Assuntos: ASTROQUÍMICA, FORMAÇÃO DE ESTRELAS

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      MENDOZA, Edgar et al. A search for cyanopolyynes in L1157-B1. Monthly Notices of the Royal Astronomical Society, v. 475, p. 5501-5512, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty180. Acesso em: 21 jul. 2024.
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      Mendoza, E., Lefloch, B., Ceccarelli, C., Kahane, C., Jaber, A. A., Polio, L., et al. (2018). A search for cyanopolyynes in L1157-B1. Monthly Notices of the Royal Astronomical Society, 475, 5501-5512. doi:10.1093/mnras/sty180
    • NLM

      Mendoza E, Lefloch B, Ceccarelli C, Kahane C, Jaber AA, Polio L, Benedettini M, Codella C, Viti S, Jimenez-Serra I, Lépine JRD, Boechat-Roberty HM, Bachiller R. A search for cyanopolyynes in L1157-B1 [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ;475 5501-5512.[citado 2024 jul. 21 ] Available from: https://doi.org/10.1093/mnras/sty180
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      Mendoza E, Lefloch B, Ceccarelli C, Kahane C, Jaber AA, Polio L, Benedettini M, Codella C, Viti S, Jimenez-Serra I, Lépine JRD, Boechat-Roberty HM, Bachiller R. A search for cyanopolyynes in L1157-B1 [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ;475 5501-5512.[citado 2024 jul. 21 ] Available from: https://doi.org/10.1093/mnras/sty180
  • Fonte: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Assuntos: GALÁXIAS, COSMOLOGIA

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      VITORELLI, André Zamorano et al. On mass concentrations and magnitude gaps of galaxy systems in the CS82 survey. Monthly Notices of the Royal Astronomical Society, v. 474, p. 866-875, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/stx2791. Acesso em: 21 jul. 2024.
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      Vitorelli, A. Z., Cypriano, E. S., Makler, M., Pereira, M. E. S., Erben, T., & Moraes, B. (2018). On mass concentrations and magnitude gaps of galaxy systems in the CS82 survey. Monthly Notices of the Royal Astronomical Society, 474, 866-875. doi:10.1093/mnras/stx2791
    • NLM

      Vitorelli AZ, Cypriano ES, Makler M, Pereira MES, Erben T, Moraes B. On mass concentrations and magnitude gaps of galaxy systems in the CS82 survey [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ;474 866-875.[citado 2024 jul. 21 ] Available from: https://doi.org/10.1093/mnras/stx2791
    • Vancouver

      Vitorelli AZ, Cypriano ES, Makler M, Pereira MES, Erben T, Moraes B. On mass concentrations and magnitude gaps of galaxy systems in the CS82 survey [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ;474 866-875.[citado 2024 jul. 21 ] Available from: https://doi.org/10.1093/mnras/stx2791
  • Fonte: Astrophysical Journal. Unidade: IAG

    Assuntos: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

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      CARLOS, Marília et al. A formation timescale of the galactic Halo from Mg isotopes in dwarf stars. Astrophysical Journal, v. 856, n. 2, p. 161-1/161-7, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aab36c. Acesso em: 21 jul. 2024.
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      Carlos, M., Karakas, A. I., Cohen, J. G., Kobayashi, C., & Moreno, J. L. M. (2018). A formation timescale of the galactic Halo from Mg isotopes in dwarf stars. Astrophysical Journal, 856( 2), 161-1/161-7. doi:10.3847/1538-4357/aab36c
    • NLM

      Carlos M, Karakas AI, Cohen JG, Kobayashi C, Moreno JLM. A formation timescale of the galactic Halo from Mg isotopes in dwarf stars [Internet]. Astrophysical Journal. 2018 ; 856( 2): 161-1/161-7.[citado 2024 jul. 21 ] Available from: https://doi.org/10.3847/1538-4357/aab36c
    • Vancouver

      Carlos M, Karakas AI, Cohen JG, Kobayashi C, Moreno JLM. A formation timescale of the galactic Halo from Mg isotopes in dwarf stars [Internet]. Astrophysical Journal. 2018 ; 856( 2): 161-1/161-7.[citado 2024 jul. 21 ] Available from: https://doi.org/10.3847/1538-4357/aab36c
  • Fonte: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. Unidade: IAG

    Assuntos: ABUNDÂNCIA ESTELAR, GALÁXIAS

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      FISHLOCK, C. K et al. Sc and neutron-capture abundances in Galactic low- and high-α field halo stars. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, v. 466, p. 4672-4682, 2017Tradução . . Disponível em: https://doi.org/10.1093/mnras/stx047. Acesso em: 21 jul. 2024.
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      Fishlock, C. K., Yong, D., Karakas, A. I., Alves-Brito, A., Moreno, J. L. M., Nissen, P. E., et al. (2017). Sc and neutron-capture abundances in Galactic low- and high-α field halo stars. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 466, 4672-4682. doi:10.1093/mnras/stx047
    • NLM

      Fishlock CK, Yong D, Karakas AI, Alves-Brito A, Moreno JLM, Nissen PE, Kobayashi C, Casey R. Sc and neutron-capture abundances in Galactic low- and high-α field halo stars [Internet]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2017 ;466 4672-4682.[citado 2024 jul. 21 ] Available from: https://doi.org/10.1093/mnras/stx047
    • Vancouver

      Fishlock CK, Yong D, Karakas AI, Alves-Brito A, Moreno JLM, Nissen PE, Kobayashi C, Casey R. Sc and neutron-capture abundances in Galactic low- and high-α field halo stars [Internet]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2017 ;466 4672-4682.[citado 2024 jul. 21 ] Available from: https://doi.org/10.1093/mnras/stx047
  • Fonte: Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. Nome do evento: IAU SYMPOSIUM. Unidade: IAG

    Assuntos: MEIO INTERESTELAR, ESTRELAS

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      CRUZ, Patricia et al. Detection of secondary eclipses of WASP-10b and Qatar-1b in the Ks band and the correlation between Ks-band temperature and stellar activity. 2017, Anais.. Cambridge: Cambridge University Press, 2017. Disponível em: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003660. Acesso em: 21 jul. 2024.
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      Cruz, P., Barrado, D., Lillo-Box, J., Diaz, M. P., López-Morales, M., Birkby, J., et al. (2017). Detection of secondary eclipses of WASP-10b and Qatar-1b in the Ks band and the correlation between Ks-band temperature and stellar activity. In Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. Cambridge: Cambridge University Press. doi:10.1017/S1743921317003660
    • NLM

      Cruz P, Barrado D, Lillo-Box J, Diaz MP, López-Morales M, Birkby J, Fortney JJ, Hodgkin S. Detection of secondary eclipses of WASP-10b and Qatar-1b in the Ks band and the correlation between Ks-band temperature and stellar activity [Internet]. Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. 2017 ;[citado 2024 jul. 21 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003660
    • Vancouver

      Cruz P, Barrado D, Lillo-Box J, Diaz MP, López-Morales M, Birkby J, Fortney JJ, Hodgkin S. Detection of secondary eclipses of WASP-10b and Qatar-1b in the Ks band and the correlation between Ks-band temperature and stellar activity [Internet]. Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. 2017 ;[citado 2024 jul. 21 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003660
  • Fonte: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. Unidade: IAG

    Assuntos: GALÁXIAS, MATÉRIA ESCURA

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      CIBIRKA, N et al. CODEX weak lensing: concentration of galaxy clusters at z ~ 0.5. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, v. 468, n. 1, p. 1092-1116, 2017Tradução . . Disponível em: https://doi.org/10.1093/mnras/stx484. Acesso em: 21 jul. 2024.
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      Cibirka, N., Cypriano, E. S., Brimioulle, F., Gruen, D., Erben, T., Van Waerbeke, L., et al. (2017). CODEX weak lensing: concentration of galaxy clusters at z ~ 0.5. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 468( 1), 1092-1116. doi:10.1093/mnras/stx484
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      Cibirka N, Cypriano ES, Brimioulle F, Gruen D, Erben T, Van Waerbeke L, Miller L, Finoguenov A, Kirkpatrick C, Henry JP, Rykoff E, Rozo E, Dupke R, Kneib J-P, Shan H, Spinelli P. CODEX weak lensing: concentration of galaxy clusters at z ~ 0.5 [Internet]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2017 ;468( 1): 1092-1116.[citado 2024 jul. 21 ] Available from: https://doi.org/10.1093/mnras/stx484
    • Vancouver

      Cibirka N, Cypriano ES, Brimioulle F, Gruen D, Erben T, Van Waerbeke L, Miller L, Finoguenov A, Kirkpatrick C, Henry JP, Rykoff E, Rozo E, Dupke R, Kneib J-P, Shan H, Spinelli P. CODEX weak lensing: concentration of galaxy clusters at z ~ 0.5 [Internet]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2017 ;468( 1): 1092-1116.[citado 2024 jul. 21 ] Available from: https://doi.org/10.1093/mnras/stx484
  • Fonte: Planetary nebulae: multi-wavelength probes of stellar and galactic evolution : proceedings of the 323rd Symposium of the International Astronomical Union held in Beijing, China, October 1-14, 2016. Nome do evento: IAU SYMPOSIUM. Unidade: IAG

    Assuntos: ABUNDÂNCIAS (ASTRONOMIA), GALÁXIA (VIA LÁCTEA)

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      MOLLÁ, Mercedes et al. The evolution of the oxygen abundance radial gradient in the Milky Way Galaxy disk. 2017, Anais.. Cambridge: Cambridge University Press, 2017. Disponível em: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317001697. Acesso em: 21 jul. 2024.
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      Mollá, M., Calvichia, O., Costa, R. D. 'A. D. da, Maciel, W. J., Gibsaon, B., & Diáz, A. I. (2017). The evolution of the oxygen abundance radial gradient in the Milky Way Galaxy disk. In Planetary nebulae: multi-wavelength probes of stellar and galactic evolution : proceedings of the 323rd Symposium of the International Astronomical Union held in Beijing, China, October 1-14, 2016. Cambridge: Cambridge University Press. doi:10.1017/S1743921317001697
    • NLM

      Mollá M, Calvichia O, Costa RD'AD da, Maciel WJ, Gibsaon B, Diáz AI. The evolution of the oxygen abundance radial gradient in the Milky Way Galaxy disk [Internet]. Planetary nebulae: multi-wavelength probes of stellar and galactic evolution : proceedings of the 323rd Symposium of the International Astronomical Union held in Beijing, China, October 1-14, 2016. 2017 ;[citado 2024 jul. 21 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317001697
    • Vancouver

      Mollá M, Calvichia O, Costa RD'AD da, Maciel WJ, Gibsaon B, Diáz AI. The evolution of the oxygen abundance radial gradient in the Milky Way Galaxy disk [Internet]. Planetary nebulae: multi-wavelength probes of stellar and galactic evolution : proceedings of the 323rd Symposium of the International Astronomical Union held in Beijing, China, October 1-14, 2016. 2017 ;[citado 2024 jul. 21 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317001697
  • Fonte: Astronomische Nachrichten. Unidade: IAG

    Assuntos: GALÁXIAS, ABUNDÂNCIA ESTELAR

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    • ABNT

      MIGLIO, A e CHIAPPINI, C e MOSSER, C. PLATO as it is: a legacy mission for Galactic archaeology. Astronomische Nachrichten, v. 338, n. 6, p. 644-661, 2017Tradução . . Disponível em: https://doi-org.ez67.periodicos.capes.gov.br/10.1002/asna.201713385. Acesso em: 21 jul. 2024.
    • APA

      Miglio, A., Chiappini, C., & Mosser, C. (2017). PLATO as it is: a legacy mission for Galactic archaeology. Astronomische Nachrichten, 338( 6), 644-661. doi:10.1002/asna.201713385
    • NLM

      Miglio A, Chiappini C, Mosser C. PLATO as it is: a legacy mission for Galactic archaeology [Internet]. Astronomische Nachrichten. 2017 ; 338( 6): 644-661.[citado 2024 jul. 21 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1002/asna.201713385
    • Vancouver

      Miglio A, Chiappini C, Mosser C. PLATO as it is: a legacy mission for Galactic archaeology [Internet]. Astronomische Nachrichten. 2017 ; 338( 6): 644-661.[citado 2024 jul. 21 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1002/asna.201713385
  • Fonte: The Astrophysical Journal. Unidade: IAG

    Assuntos: CATÁLOGOS, GALÁXIAS, ABUNDÂNCIAS (ASTRONOMIA), GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR, POPULAÇÕES ESTELARES, ESTRELAS, CARBONO, ESPECTROSCOPIA

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    • ABNT

      BEERS, Timothy C et al. Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis. The Astrophysical Journal, v. 835, p. 81, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/835/1/81. Acesso em: 21 jul. 2024.
    • APA

      Beers, T. C., Placco, V. M., Carollo, D., Rossi, S. C. F., Lee, Y. S., Frebel, A., et al. (2017). Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis. The Astrophysical Journal, 835, 81. doi:10.3847/1538-4357/835/1/81
    • NLM

      Beers TC, Placco VM, Carollo D, Rossi SCF, Lee YS, Frebel A, Norris JE, Dietz S, Masseron T. Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis [Internet]. The Astrophysical Journal. 2017 ; 835 81.[citado 2024 jul. 21 ] Available from: https://doi.org/10.3847/1538-4357/835/1/81
    • Vancouver

      Beers TC, Placco VM, Carollo D, Rossi SCF, Lee YS, Frebel A, Norris JE, Dietz S, Masseron T. Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis [Internet]. The Astrophysical Journal. 2017 ; 835 81.[citado 2024 jul. 21 ] Available from: https://doi.org/10.3847/1538-4357/835/1/81
  • Fonte: Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. Nome do evento: IAU SYMPOSIUM. Unidade: IAG

    Assuntos: ESTRELAS, ASTROFÍSICA ESTELAR

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      GUERRERO, G et al. Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations. 2017, Anais.. Cambridge: Cambridge University Press, 2017. Disponível em: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003982. Acesso em: 21 jul. 2024.
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      Guerrero, G., Smolarkiewicz, P. K., Gouveia dal Pino, E. M. de, Kososichev, A. G., Zaire, B., & Mansour, N. N. (2017). Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations. In Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. Cambridge: Cambridge University Press. doi:10.1017/S1743921317003982
    • NLM

      Guerrero G, Smolarkiewicz PK, Gouveia dal Pino EM de, Kososichev AG, Zaire B, Mansour NN. Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations [Internet]. Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. 2017 ;[citado 2024 jul. 21 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003982
    • Vancouver

      Guerrero G, Smolarkiewicz PK, Gouveia dal Pino EM de, Kososichev AG, Zaire B, Mansour NN. Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations [Internet]. Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. 2017 ;[citado 2024 jul. 21 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003982
  • Fonte: Astrophysical Journal. Unidade: IAG

    Assuntos: GALÁXIAS, ABUNDÂNCIA ESTELAR

    Acesso à fonteDOIComo citar
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    • ABNT

      BEERS, Timothy C et al. Bight metal-poor stars from the Hamburg/ESO survey. II. A chemodynamical analysis. Astrophysical Journal, v. 835, n. 1, p. 81, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/835/1/81. Acesso em: 21 jul. 2024.
    • APA

      Beers, T. C., Placco, V. M., Carollo, D., Rossi, S. C. F., Lee, Y. S., Frebel, A., et al. (2017). Bight metal-poor stars from the Hamburg/ESO survey. II. A chemodynamical analysis. Astrophysical Journal, 835( 1), 81. doi:10.3847/1538-4357/835/1/81
    • NLM

      Beers TC, Placco VM, Carollo D, Rossi SCF, Lee YS, Frebel A, Norris JE, Dietz S, Masseron T. Bight metal-poor stars from the Hamburg/ESO survey. II. A chemodynamical analysis [Internet]. Astrophysical Journal. 2017 ;835( 1): 81.[citado 2024 jul. 21 ] Available from: https://doi.org/10.3847/1538-4357/835/1/81
    • Vancouver

      Beers TC, Placco VM, Carollo D, Rossi SCF, Lee YS, Frebel A, Norris JE, Dietz S, Masseron T. Bight metal-poor stars from the Hamburg/ESO survey. II. A chemodynamical analysis [Internet]. Astrophysical Journal. 2017 ;835( 1): 81.[citado 2024 jul. 21 ] Available from: https://doi.org/10.3847/1538-4357/835/1/81
  • Fonte: Astrophysical Journal Letters. Unidade: IAG

    Assuntos: SOL, CAMPO MAGNÉTICO

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    • ABNT

      GUERRERO, G e SMOLARKIEWICZ, P. K e DAL PINO, Elisabete Maria de Gouveia. Understanding solar torsional oscillations from global dynamo models. Astrophysical Journal Letters, 2016Tradução . . Disponível em: https://arxiv.org/abs/1608.02278. Acesso em: 21 jul. 2024.
    • APA

      Guerrero, G., Smolarkiewicz, P. K., & Dal Pino, E. M. de G. (2016). Understanding solar torsional oscillations from global dynamo models. Astrophysical Journal Letters. doi:10.3847/2041-8205/828/1/L3
    • NLM

      Guerrero G, Smolarkiewicz PK, Dal Pino EM de G. Understanding solar torsional oscillations from global dynamo models [Internet]. Astrophysical Journal Letters. 2016 ;[citado 2024 jul. 21 ] Available from: https://arxiv.org/abs/1608.02278
    • Vancouver

      Guerrero G, Smolarkiewicz PK, Dal Pino EM de G. Understanding solar torsional oscillations from global dynamo models [Internet]. Astrophysical Journal Letters. 2016 ;[citado 2024 jul. 21 ] Available from: https://arxiv.org/abs/1608.02278

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