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  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ASTROQUÍMICA, ABUNDÂNCIA ESTELAR, JATOS (ASTRONOMIA)

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      DURONEA, N. U et al. Cyanoacetylene in the outflow/hot molecular core G331.512-0.103. Monthly Notices of the Royal Astronomical Society, v. 489, n. 2, p. 1519-1532, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz2087. Acesso em: 03 maio 2024.
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      Duronea, N. U., Bronfman, L., Mendoza, E., Merello, M., Finger, R., Reyes, N., et al. (2019). Cyanoacetylene in the outflow/hot molecular core G331.512-0.103. Monthly Notices of the Royal Astronomical Society, 489( 2), 1519-1532. doi:10.1093/mnras/stz2087
    • NLM

      Duronea NU, Bronfman L, Mendoza E, Merello M, Finger R, Reyes N, Hervias-Caimapo C, Faure A, Cappa CE, Arnal EM, Lépine JRD, Kleiner I, Nyman L-A. Cyanoacetylene in the outflow/hot molecular core G331.512-0.103 [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 489( 2): 1519-1532.[citado 2024 maio 03 ] Available from: https://doi.org/10.1093/mnras/stz2087
    • Vancouver

      Duronea NU, Bronfman L, Mendoza E, Merello M, Finger R, Reyes N, Hervias-Caimapo C, Faure A, Cappa CE, Arnal EM, Lépine JRD, Kleiner I, Nyman L-A. Cyanoacetylene in the outflow/hot molecular core G331.512-0.103 [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 489( 2): 1519-1532.[citado 2024 maio 03 ] Available from: https://doi.org/10.1093/mnras/stz2087
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ESTRELAS BINARIAS

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      RAMIREZ, et al. The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs. Monthly Notices of the Royal Astronomical Society, v. 490, p. 2448-2457, 2019Tradução . . Disponível em: https://academic.oup.com/mnras/article/490/2/2448/5583050. Acesso em: 03 maio 2024.
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      Ramirez,, Khanal, S., Lichon, S. J., Chanamé, J., Endl, M., Moreno, J. L. M., & Lambert, D. L. (2019). The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs. Monthly Notices of the Royal Astronomical Society, 490, 2448-2457. doi:10.1093/mnras/sty104
    • NLM

      Ramirez, Khanal S, Lichon SJ, Chanamé J, Endl M, Moreno JLM, Lambert DL. The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 2448-2457.[citado 2024 maio 03 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
    • Vancouver

      Ramirez, Khanal S, Lichon SJ, Chanamé J, Endl M, Moreno JLM, Lambert DL. The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 2448-2457.[citado 2024 maio 03 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, GALÁXIAS ELÍPTICAS, ESTRUTURA DA GALÁXIA

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      BARBOSA, C. E et al. Sloshing in its cD halo: MUSE kinematics of the central galaxy NGC 3311 in the Hydra I cluster. Astronomy & Astrophysics, v. 609, p. A78, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201731834. Acesso em: 03 maio 2024.
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      Barbosa, C. E., Arnaboldi, M., Coccato, L., Gerhard, O., Oliveira, C. L. M. de, Hilker, M., & Richtler, T. (2018). Sloshing in its cD halo: MUSE kinematics of the central galaxy NGC 3311 in the Hydra I cluster. Astronomy & Astrophysics, 609, A78. doi:10.1051/0004-6361/201731834
    • NLM

      Barbosa CE, Arnaboldi M, Coccato L, Gerhard O, Oliveira CLM de, Hilker M, Richtler T. Sloshing in its cD halo: MUSE kinematics of the central galaxy NGC 3311 in the Hydra I cluster [Internet]. Astronomy & Astrophysics. 2018 ; 609 A78.[citado 2024 maio 03 ] Available from: https://doi.org/10.1051/0004-6361/201731834
    • Vancouver

      Barbosa CE, Arnaboldi M, Coccato L, Gerhard O, Oliveira CLM de, Hilker M, Richtler T. Sloshing in its cD halo: MUSE kinematics of the central galaxy NGC 3311 in the Hydra I cluster [Internet]. Astronomy & Astrophysics. 2018 ; 609 A78.[citado 2024 maio 03 ] Available from: https://doi.org/10.1051/0004-6361/201731834
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: FOTOMETRIA, ESTRELAS, DISCOS DE ACRESÇÃO

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      GHOREYSHI, M. R et al. The life cycles of Be viscous decretion discs: The case of ω CMa. Monthly Notices of the Royal Astronomical Society, v. 479, p. 2214-2228, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty1577. Acesso em: 03 maio 2024.
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      Ghoreyshi, M. R., Carciofi, A. C., Rímulo, L. R., Vieria, R. G., Faes, D. M., Baade, D., et al. (2018). The life cycles of Be viscous decretion discs: The case of ω CMa. Monthly Notices of the Royal Astronomical Society, 479, 2214-2228. doi:10.1093/mnras/sty1577
    • NLM

      Ghoreyshi MR, Carciofi AC, Rímulo LR, Vieria RG, Faes DM, Baade D, Bjorkman JE, Otero S, Rivinius T. The life cycles of Be viscous decretion discs: The case of ω CMa [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 479 2214-2228.[citado 2024 maio 03 ] Available from: https://doi.org/10.1093/mnras/sty1577
    • Vancouver

      Ghoreyshi MR, Carciofi AC, Rímulo LR, Vieria RG, Faes DM, Baade D, Bjorkman JE, Otero S, Rivinius T. The life cycles of Be viscous decretion discs: The case of ω CMa [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 479 2214-2228.[citado 2024 maio 03 ] Available from: https://doi.org/10.1093/mnras/sty1577
  • Source: The Astrophysical Journal. Unidade: IAG

    Assunto: MEIO INTERESTELAR

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      MENDOZA, Edgar et al. G331.512-0.103: An Interstellar Laboratory for Molecular Synthesis I. The Ortho-to-para Ratios for CH3OH and CH3CN. The Astrophysical Journal, v. 853, p. 152, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aaa1ec. Acesso em: 03 maio 2024.
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      Mendoza, E., Bronfman, L., Duronea, N. U., Lépine, J. R. D., Finger, R., Merello, M., et al. (2018). G331.512-0.103: An Interstellar Laboratory for Molecular Synthesis I. The Ortho-to-para Ratios for CH3OH and CH3CN. The Astrophysical Journal, 853, 152. doi:10.3847/1538-4357/aaa1ec
    • NLM

      Mendoza E, Bronfman L, Duronea NU, Lépine JRD, Finger R, Merello M, Caimapo CH, Gama DRG, Ake-Nyman L. G331.512-0.103: An Interstellar Laboratory for Molecular Synthesis I. The Ortho-to-para Ratios for CH3OH and CH3CN [Internet]. The Astrophysical Journal. 2018 ; 853 152.[citado 2024 maio 03 ] Available from: https://doi.org/10.3847/1538-4357/aaa1ec
    • Vancouver

      Mendoza E, Bronfman L, Duronea NU, Lépine JRD, Finger R, Merello M, Caimapo CH, Gama DRG, Ake-Nyman L. G331.512-0.103: An Interstellar Laboratory for Molecular Synthesis I. The Ortho-to-para Ratios for CH3OH and CH3CN [Internet]. The Astrophysical Journal. 2018 ; 853 152.[citado 2024 maio 03 ] Available from: https://doi.org/10.3847/1538-4357/aaa1ec
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, POPULAÇÕES ESTELARES, ESTRELAS

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      HILKER, M et al. The Hydra I cluster core: II. Kinematic complexity in a rising velocity dispersion profile around the cD galaxy NGC 3311. Astronomy & Astrophysics, v. 619, p. A70, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201731737. Acesso em: 03 maio 2024.
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      Hilker, M., Richtler, T., Barbosa, C. E., Arnaboldi, M., Coccato, L., & Oliveira, C. M. de. (2018). The Hydra I cluster core: II. Kinematic complexity in a rising velocity dispersion profile around the cD galaxy NGC 3311. Astronomy & Astrophysics, 619, A70. doi:10.1051/0004-6361/201731737
    • NLM

      Hilker M, Richtler T, Barbosa CE, Arnaboldi M, Coccato L, Oliveira CM de. The Hydra I cluster core: II. Kinematic complexity in a rising velocity dispersion profile around the cD galaxy NGC 3311 [Internet]. Astronomy & Astrophysics. 2018 ;619 A70.[citado 2024 maio 03 ] Available from: https://doi.org/10.1051/0004-6361/201731737
    • Vancouver

      Hilker M, Richtler T, Barbosa CE, Arnaboldi M, Coccato L, Oliveira CM de. The Hydra I cluster core: II. Kinematic complexity in a rising velocity dispersion profile around the cD galaxy NGC 3311 [Internet]. Astronomy & Astrophysics. 2018 ;619 A70.[citado 2024 maio 03 ] Available from: https://doi.org/10.1051/0004-6361/201731737
  • Source: Astronomy & Astrophysics. Unidade: IAG

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

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      BARBUY, Beatriz Leonor Silveira et al. High-resolution abundance analysis of four red giants in the globular cluster NGC 6558. Astronomy & Astrophysics, v. 619, p. A178, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201833953. Acesso em: 03 maio 2024.
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      Barbuy, B. L. S., Muniz, L., Ortolani, S., Ernandes, H., Dias, B., Saviane, I., et al. (2018). High-resolution abundance analysis of four red giants in the globular cluster NGC 6558. Astronomy & Astrophysics, 619, A178. doi:10.1051/0004-6361/201833953
    • NLM

      Barbuy BLS, Muniz L, Ortolani S, Ernandes H, Dias B, Saviane I, Kerber L, Bica E, Pérez-Villegas A, Rossi L, Held EV. High-resolution abundance analysis of four red giants in the globular cluster NGC 6558 [Internet]. Astronomy & Astrophysics. 2018 ; 619 A178.[citado 2024 maio 03 ] Available from: https://doi.org/10.1051/0004-6361/201833953
    • Vancouver

      Barbuy BLS, Muniz L, Ortolani S, Ernandes H, Dias B, Saviane I, Kerber L, Bica E, Pérez-Villegas A, Rossi L, Held EV. High-resolution abundance analysis of four red giants in the globular cluster NGC 6558 [Internet]. Astronomy & Astrophysics. 2018 ; 619 A178.[citado 2024 maio 03 ] Available from: https://doi.org/10.1051/0004-6361/201833953
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES

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      SPINA, Lorenzo et al. Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres. Astrophysical Journal, v. 863, n. 2, p. 179-1/179-6, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad190. Acesso em: 03 maio 2024.
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      Spina, L., Moreno, J. L. M., Casey, A. R., Karakas, A. I., & Tucci-Maia, M. (2018). Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres. Astrophysical Journal, 863( 2), 179-1/179-6. doi:10.3847/1538-4357/aad190
    • NLM

      Spina L, Moreno JLM, Casey AR, Karakas AI, Tucci-Maia M. Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres [Internet]. Astrophysical Journal. 2018 ; 863( 2): 179-1/179-6.[citado 2024 maio 03 ] Available from: https://doi.org/10.3847/1538-4357/aad190
    • Vancouver

      Spina L, Moreno JLM, Casey AR, Karakas AI, Tucci-Maia M. Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres [Internet]. Astrophysical Journal. 2018 ; 863( 2): 179-1/179-6.[citado 2024 maio 03 ] Available from: https://doi.org/10.3847/1538-4357/aad190
  • Source: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. Unidade: IAG

    Subjects: HIDRODINÂMICA, ESTRELAS BINÁRIAS

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      PANOGLOU, Despina et al. Be discs in coplanar circular binaries: Phase-locked variations of emission lines. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, v. 473, p. 3039-3050, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/stx2497. Acesso em: 03 maio 2024.
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      Panoglou, D., Faes, D. M., Carciofi, A. C., Okazaki, A. T., Baade, D., Rivinius, T., & Fernandes, M. B. (2018). Be discs in coplanar circular binaries: Phase-locked variations of emission lines. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 473, 3039-3050. doi:10.1093/mnras/stx2497
    • NLM

      Panoglou D, Faes DM, Carciofi AC, Okazaki AT, Baade D, Rivinius T, Fernandes MB. Be discs in coplanar circular binaries: Phase-locked variations of emission lines [Internet]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2018 ;473 3039-3050.[citado 2024 maio 03 ] Available from: https://doi.org/10.1093/mnras/stx2497
    • Vancouver

      Panoglou D, Faes DM, Carciofi AC, Okazaki AT, Baade D, Rivinius T, Fernandes MB. Be discs in coplanar circular binaries: Phase-locked variations of emission lines [Internet]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2018 ;473 3039-3050.[citado 2024 maio 03 ] Available from: https://doi.org/10.1093/mnras/stx2497
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: HIDRODINÂMICA, FOTOMETRIA

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      RIMULO, L. R et al. The life cycles of Be viscous decretion discs: fundamental disc parameters of 54 SMC Be stars. Monthly Notices of the Royal Astronomical Society, v. 476, p. 3555-3579, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty431. Acesso em: 03 maio 2024.
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      Rimulo, L. R., Carciofi, A. C., Vieira, R. G., Rivinius, T., Faes, D. M., Figueiredo, A. L., et al. (2018). The life cycles of Be viscous decretion discs: fundamental disc parameters of 54 SMC Be stars. Monthly Notices of the Royal Astronomical Society, 476, 3555-3579. doi:10.1093/mnras/sty431
    • NLM

      Rimulo LR, Carciofi AC, Vieira RG, Rivinius T, Faes DM, Figueiredo AL, Bjorkman JE, Georgy C, Ghoreyshi MR, Soszynski I. The life cycles of Be viscous decretion discs: fundamental disc parameters of 54 SMC Be stars [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 476 3555-3579.[citado 2024 maio 03 ] Available from: https://doi.org/10.1093/mnras/sty431
    • Vancouver

      Rimulo LR, Carciofi AC, Vieira RG, Rivinius T, Faes DM, Figueiredo AL, Bjorkman JE, Georgy C, Ghoreyshi MR, Soszynski I. The life cycles of Be viscous decretion discs: fundamental disc parameters of 54 SMC Be stars [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 476 3555-3579.[citado 2024 maio 03 ] Available from: https://doi.org/10.1093/mnras/sty431
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: DINÂMICA DAS GALÁXIAS, GALÁXIAS

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      MUÑOZ-ELGUETA, N et al. Kinematics and physical properties of the nearby galaxy NGC 4656 and its TDG candidate. Monthly Notices of the Royal Astronomical Society, v. 480, n. 3, p. 3257-3278, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty1934. Acesso em: 03 maio 2024.
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      Muñoz-Elgueta, N., Torres-Flores, S., Amram, P., Hernandez-Jimenez, J. A., Urrutia-Viscarra, F., Oliveira, C. L. M. de, & Gómez-López, A. (2018). Kinematics and physical properties of the nearby galaxy NGC 4656 and its TDG candidate. Monthly Notices of the Royal Astronomical Society, 480( 3), 3257-3278. doi:10.1093/mnras/sty1934
    • NLM

      Muñoz-Elgueta N, Torres-Flores S, Amram P, Hernandez-Jimenez JA, Urrutia-Viscarra F, Oliveira CLM de, Gómez-López A. Kinematics and physical properties of the nearby galaxy NGC 4656 and its TDG candidate [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 480( 3): 3257-3278.[citado 2024 maio 03 ] Available from: https://doi.org/10.1093/mnras/sty1934
    • Vancouver

      Muñoz-Elgueta N, Torres-Flores S, Amram P, Hernandez-Jimenez JA, Urrutia-Viscarra F, Oliveira CLM de, Gómez-López A. Kinematics and physical properties of the nearby galaxy NGC 4656 and its TDG candidate [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 480( 3): 3257-3278.[citado 2024 maio 03 ] Available from: https://doi.org/10.1093/mnras/sty1934
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ESPECTROSCOPIA, ASTROFÍSICA ESTELAR

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      CHOJNOWSKI, S. Drew et al. The remarkable Be+sdOB Binary HD 55606. I. Orbital and stellar parameters. Astrophysical Journal, v. 865, n. 1, p. 76-1/76-16, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad964. Acesso em: 03 maio 2024.
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      Chojnowski, S. D., Labadie-Bartz, J., Rivinius, T., Gies, D., & Leister, N. V. (2018). The remarkable Be+sdOB Binary HD 55606. I. Orbital and stellar parameters. Astrophysical Journal, 865( 1), 76-1/76-16. doi:10.3847/1538-4357/aad964
    • NLM

      Chojnowski SD, Labadie-Bartz J, Rivinius T, Gies D, Leister NV. The remarkable Be+sdOB Binary HD 55606. I. Orbital and stellar parameters [Internet]. Astrophysical Journal. 2018 ; 865( 1): 76-1/76-16.[citado 2024 maio 03 ] Available from: https://doi.org/10.3847/1538-4357/aad964
    • Vancouver

      Chojnowski SD, Labadie-Bartz J, Rivinius T, Gies D, Leister NV. The remarkable Be+sdOB Binary HD 55606. I. Orbital and stellar parameters [Internet]. Astrophysical Journal. 2018 ; 865( 1): 76-1/76-16.[citado 2024 maio 03 ] Available from: https://doi.org/10.3847/1538-4357/aad964
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS, FOTOMETRIA

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      BAADE, Dietrich et al. Short-term variability and mass loss in Be stars: III. BRITE and SMEI satellite photometry of 28 Cygni★,★★. Astronomy & Astrophysics, v. 610, n. A70 p. 17p, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201731187. Acesso em: 03 maio 2024.
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      Baade, D., Pigulski, A., Rivinius, T., Carciofi, A. C., Panoglou, D., Ghoreyshi, M. R., et al. (2018). Short-term variability and mass loss in Be stars: III. BRITE and SMEI satellite photometry of 28 Cygni★,★★. Astronomy & Astrophysics, 610( A70 p. 17p). doi:10.1051/0004-6361/201731187
    • NLM

      Baade D, Pigulski A, Rivinius T, Carciofi AC, Panoglou D, Ghoreyshi MR, Handler G, Kuschnig R, Moffat AFJ, Pablo H, Popowicz A, Wade GA, Weiss WW, Zwintz K. Short-term variability and mass loss in Be stars: III. BRITE and SMEI satellite photometry of 28 Cygni★,★★ [Internet]. Astronomy & Astrophysics. 2018 ; 610( A70 p. 17p):[citado 2024 maio 03 ] Available from: https://doi.org/10.1051/0004-6361/201731187
    • Vancouver

      Baade D, Pigulski A, Rivinius T, Carciofi AC, Panoglou D, Ghoreyshi MR, Handler G, Kuschnig R, Moffat AFJ, Pablo H, Popowicz A, Wade GA, Weiss WW, Zwintz K. Short-term variability and mass loss in Be stars: III. BRITE and SMEI satellite photometry of 28 Cygni★,★★ [Internet]. Astronomy & Astrophysics. 2018 ; 610( A70 p. 17p):[citado 2024 maio 03 ] Available from: https://doi.org/10.1051/0004-6361/201731187
  • Source: Geoscientific Model Development. Unidade: IAG

    Subjects: METEOROLOGIA AMBIENTAL, POLUIÇÃO ATMOSFÉRICA, VEÍCULOS AUTOMOTORES

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      IBARRA-ESPINOSA, Sergio et al. VEIN v0.2.2: an R package for bottom–up vehicular emissions inventories. Geoscientific Model Development, v. 11, n. 6, p. 2209-2229, 2018Tradução . . Disponível em: https://doi.org/10.5194/gmd-11-2209-2018. Acesso em: 03 maio 2024.
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      Ibarra-Espinosa, S., Ynoue, R. Y., O'Sullivan, S., Pebesma, E., Andrade, M. de F., & Osses, M. (2018). VEIN v0.2.2: an R package for bottom–up vehicular emissions inventories. Geoscientific Model Development, 11( 6), 2209-2229. doi:10.5194/gmd-11-2209-2018
    • NLM

      Ibarra-Espinosa S, Ynoue RY, O'Sullivan S, Pebesma E, Andrade M de F, Osses M. VEIN v0.2.2: an R package for bottom–up vehicular emissions inventories [Internet]. Geoscientific Model Development. 2018 ; 11( 6): 2209-2229.[citado 2024 maio 03 ] Available from: https://doi.org/10.5194/gmd-11-2209-2018
    • Vancouver

      Ibarra-Espinosa S, Ynoue RY, O'Sullivan S, Pebesma E, Andrade M de F, Osses M. VEIN v0.2.2: an R package for bottom–up vehicular emissions inventories [Internet]. Geoscientific Model Development. 2018 ; 11( 6): 2209-2229.[citado 2024 maio 03 ] Available from: https://doi.org/10.5194/gmd-11-2209-2018
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Assunto: GALÁXIAS

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      MACHADO, R. E. G et al. Properties of the circumgalactic medium in simulations compared to observations. Astronomy & Astrophysics, v. 609, n. A66, p. 15 , 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201628886. Acesso em: 03 maio 2024.
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      Machado, R. E. G., Tissera, P. B., Lima Neto, G. C. B., & Sodré Júnior, L. (2018). Properties of the circumgalactic medium in simulations compared to observations. Astronomy & Astrophysics, 609( A66), 15 . doi:10.1051/0004-6361/201628886
    • NLM

      Machado REG, Tissera PB, Lima Neto GCB, Sodré Júnior L. Properties of the circumgalactic medium in simulations compared to observations [Internet]. Astronomy & Astrophysics. 2018 ; 609( A66): 15 .[citado 2024 maio 03 ] Available from: https://doi.org/10.1051/0004-6361/201628886
    • Vancouver

      Machado REG, Tissera PB, Lima Neto GCB, Sodré Júnior L. Properties of the circumgalactic medium in simulations compared to observations [Internet]. Astronomy & Astrophysics. 2018 ; 609( A66): 15 .[citado 2024 maio 03 ] Available from: https://doi.org/10.1051/0004-6361/201628886
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR, GALÁXIA (VIA LÁCTEA)

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      VÁSQUEZ, S et al. Homogeneous metallicities and radial velocities for Galactic globular clusters: II. New CaT metallicities for 28 distant and reddened globular clusters. Astronomy & Astrophysics, v. 619, p. A13, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201833525. Acesso em: 03 maio 2024.
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      Vásquez, S., Saviane, I., Held, E. V., Da Costa, G. S., Dias, B., Gullieuszik, M., et al. (2018). Homogeneous metallicities and radial velocities for Galactic globular clusters: II. New CaT metallicities for 28 distant and reddened globular clusters. Astronomy & Astrophysics, 619, A13. doi:10.1051/0004-6361/201833525
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      Vásquez S, Saviane I, Held EV, Da Costa GS, Dias B, Gullieuszik M, Barbuy BLS, Ortolani S, Zoccali M. Homogeneous metallicities and radial velocities for Galactic globular clusters: II. New CaT metallicities for 28 distant and reddened globular clusters [Internet]. Astronomy & Astrophysics. 2018 ; 619 A13.[citado 2024 maio 03 ] Available from: https://doi.org/10.1051/0004-6361/201833525
    • Vancouver

      Vásquez S, Saviane I, Held EV, Da Costa GS, Dias B, Gullieuszik M, Barbuy BLS, Ortolani S, Zoccali M. Homogeneous metallicities and radial velocities for Galactic globular clusters: II. New CaT metallicities for 28 distant and reddened globular clusters [Internet]. Astronomy & Astrophysics. 2018 ; 619 A13.[citado 2024 maio 03 ] Available from: https://doi.org/10.1051/0004-6361/201833525
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, GALÁXIAS

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      SILVEIRA, C. R. da et al. Oxygen and zinc abundances in 417 Galactic bulge red giants★. Astronomy & Astrophysics, v. 614, p. A149, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201730562. Acesso em: 03 maio 2024.
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      Silveira, C. R. da, Barbuy, B. L. S., Friaça, A. C. S., Hill, V., Zoccali, M., Rafelski, S., et al. (2018). Oxygen and zinc abundances in 417 Galactic bulge red giants★. Astronomy & Astrophysics, 614, A149. doi:10.1051/0004-6361/201730562
    • NLM

      Silveira CR da, Barbuy BLS, Friaça ACS, Hill V, Zoccali M, Rafelski S, González OA, Minniti D, Renzini A, Ortolani S. Oxygen and zinc abundances in 417 Galactic bulge red giants★ [Internet]. Astronomy & Astrophysics. 2018 ; 614 A149.[citado 2024 maio 03 ] Available from: https://doi.org/10.1051/0004-6361/201730562
    • Vancouver

      Silveira CR da, Barbuy BLS, Friaça ACS, Hill V, Zoccali M, Rafelski S, González OA, Minniti D, Renzini A, Ortolani S. Oxygen and zinc abundances in 417 Galactic bulge red giants★ [Internet]. Astronomy & Astrophysics. 2018 ; 614 A149.[citado 2024 maio 03 ] Available from: https://doi.org/10.1051/0004-6361/201730562
  • Source: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. Unidade: IAG

    Subjects: ABUNDÂNCIAS (ASTRONOMIA), ESTRELAS

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      PULS, Arthur A et al. Chemical analysis of eight giant stars of the globular cluster NGC 6366. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, v. 476, p. 690-704, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty267. Acesso em: 03 maio 2024.
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      Puls, A. A., Brito, A. A., Campos, F., Dias, B., & Barbuy, B. L. S. (2018). Chemical analysis of eight giant stars of the globular cluster NGC 6366. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 476, 690-704. doi:10.1093/mnras/sty267
    • NLM

      Puls AA, Brito AA, Campos F, Dias B, Barbuy BLS. Chemical analysis of eight giant stars of the globular cluster NGC 6366 [Internet]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2018 ;476 690-704.[citado 2024 maio 03 ] Available from: https://doi.org/10.1093/mnras/sty267
    • Vancouver

      Puls AA, Brito AA, Campos F, Dias B, Barbuy BLS. Chemical analysis of eight giant stars of the globular cluster NGC 6366 [Internet]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2018 ;476 690-704.[citado 2024 maio 03 ] Available from: https://doi.org/10.1093/mnras/sty267
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS, FOTOMETRIA

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      BAADE, D et al. Short-term variability and mass loss in Be stars: IV. Two groups of closely spaced, approximately equidistant frequencies in three decades of space photometry of ν Puppis (B7-8 IIIe). Astronomy & Astrophysics, v. 620, p. A145, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201834161. Acesso em: 03 maio 2024.
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      Baade, D., Pigulski, A., Rivinius, T., Wang, L., Martayan, C., Handler, G., et al. (2018). Short-term variability and mass loss in Be stars: IV. Two groups of closely spaced, approximately equidistant frequencies in three decades of space photometry of ν Puppis (B7-8 IIIe). Astronomy & Astrophysics, 620, A145. doi:10.1051/0004-6361/201834161
    • NLM

      Baade D, Pigulski A, Rivinius T, Wang L, Martayan C, Handler G, Panoglou D, Carciofi AC, Kuschnig R, Mehner A, Moffat AFJ, Pablo H, Rucinski SM, Wade GA, Weiss WW, Zwintz K. Short-term variability and mass loss in Be stars: IV. Two groups of closely spaced, approximately equidistant frequencies in three decades of space photometry of ν Puppis (B7-8 IIIe) [Internet]. Astronomy & Astrophysics. 2018 ; 620 A145.[citado 2024 maio 03 ] Available from: https://doi.org/10.1051/0004-6361/201834161
    • Vancouver

      Baade D, Pigulski A, Rivinius T, Wang L, Martayan C, Handler G, Panoglou D, Carciofi AC, Kuschnig R, Mehner A, Moffat AFJ, Pablo H, Rucinski SM, Wade GA, Weiss WW, Zwintz K. Short-term variability and mass loss in Be stars: IV. Two groups of closely spaced, approximately equidistant frequencies in three decades of space photometry of ν Puppis (B7-8 IIIe) [Internet]. Astronomy & Astrophysics. 2018 ; 620 A145.[citado 2024 maio 03 ] Available from: https://doi.org/10.1051/0004-6361/201834161
  • Source: The B[e] phenomenon: forty years of studies. Conference titles: Proceedings of a conference held at Charles University. Unidade: IAG

    Subjects: ASTROFÍSICA ESTELAR, DISCOS DE ACRESÇÃO

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      VIEIRA, R. G et al. The viscous decretion disc properties of 80 Be stars. 2017, Anais.. San Francico: Astronomical Society of the Pacific, 2017. . Acesso em: 03 maio 2024.
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      Vieira, R. G., Baade, D., Rímulo, L. R., Carciofi, A. C., Bjorkman, J. E., & Rivinius, T. (2017). The viscous decretion disc properties of 80 Be stars. In The B[e] phenomenon: forty years of studies. San Francico: Astronomical Society of the Pacific.
    • NLM

      Vieira RG, Baade D, Rímulo LR, Carciofi AC, Bjorkman JE, Rivinius T. The viscous decretion disc properties of 80 Be stars. The B[e] phenomenon: forty years of studies. 2017 ;[citado 2024 maio 03 ]
    • Vancouver

      Vieira RG, Baade D, Rímulo LR, Carciofi AC, Bjorkman JE, Rivinius T. The viscous decretion disc properties of 80 Be stars. The B[e] phenomenon: forty years of studies. 2017 ;[citado 2024 maio 03 ]

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