Filtros : "ABUNDÂNCIA ESTELAR" "Chile" Removidos: "IMPARATO, JOSE CARLOS PETTOROSSI" "2020-2022" "20212" Limpar

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  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ABUNDÂNCIA ESTELAR

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      FERNÁNDEZ-TRINCADO, D. G et al. H-band discovery of additional second-generation stars in the Galactic bulge globular cluster NGC 6522 as observed by APOGEE and Gaia. Astronomy & Astrophysics, v. 627, p. A178, 2019Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201834391. Acesso em: 20 ago. 2024.
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      Fernández-Trincado, D. G., Schiavon, R. P., Almeida, A. A. de, & Roman-Lopes, A. (2019). H-band discovery of additional second-generation stars in the Galactic bulge globular cluster NGC 6522 as observed by APOGEE and Gaia. Astronomy & Astrophysics, 627, A178. doi:10.1051/0004-6361/201834391
    • NLM

      Fernández-Trincado DG, Schiavon RP, Almeida AA de, Roman-Lopes A. H-band discovery of additional second-generation stars in the Galactic bulge globular cluster NGC 6522 as observed by APOGEE and Gaia [Internet]. Astronomy & Astrophysics. 2019 ; 627 A178.[citado 2024 ago. 20 ] Available from: https://doi.org/10.1051/0004-6361/201834391
    • Vancouver

      Fernández-Trincado DG, Schiavon RP, Almeida AA de, Roman-Lopes A. H-band discovery of additional second-generation stars in the Galactic bulge globular cluster NGC 6522 as observed by APOGEE and Gaia [Internet]. Astronomy & Astrophysics. 2019 ; 627 A178.[citado 2024 ago. 20 ] Available from: https://doi.org/10.1051/0004-6361/201834391
  • 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: 20 ago. 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 ago. 20 ] 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 ago. 20 ] 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: 20 ago. 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 ago. 20 ] 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 ago. 20 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
  • Source: Astronomy & Astrophysics. Unidade: IAG

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

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    • ABNT

      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: 20 ago. 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 ago. 20 ] 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 ago. 20 ] Available from: https://doi.org/10.1051/0004-6361/201833953
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES

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    • ABNT

      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: 20 ago. 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 ago. 20 ] 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 ago. 20 ] Available from: https://doi.org/10.3847/1538-4357/aad190
  • 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: 20 ago. 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
    • NLM

      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 ago. 20 ] 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 ago. 20 ] 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: 20 ago. 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 ago. 20 ] 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 ago. 20 ] Available from: https://doi.org/10.1051/0004-6361/201730562
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ESPECTROSCOPIA

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      THYGESEN, A. O et al. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios. Astronomy & Astrophysics, v. 590, p. A66/1-A66/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201526643. Acesso em: 20 ago. 2024.
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      Thygesen, A. O., Sbordone, L., Ludwig, H. -G., Ventura, P., Yong, D., Collet, R., et al. (2016). The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios. Astronomy & Astrophysics, 590, A66/1-A66/8. doi:10.1051/0004-6361/201526643
    • NLM

      Thygesen AO, Sbordone L, Ludwig H-G, Ventura P, Yong D, Collet R, Christlieb N, Moreno JLM, Zaggia S. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios [Internet]. Astronomy & Astrophysics. 2016 ; 590 A66/1-A66/8.[citado 2024 ago. 20 ] Available from: https://doi.org/10.1051/0004-6361/201526643
    • Vancouver

      Thygesen AO, Sbordone L, Ludwig H-G, Ventura P, Yong D, Collet R, Christlieb N, Moreno JLM, Zaggia S. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios [Internet]. Astronomy & Astrophysics. 2016 ; 590 A66/1-A66/8.[citado 2024 ago. 20 ] Available from: https://doi.org/10.1051/0004-6361/201526643
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, DINÂMICA, CINEMÁTICA, POPULAÇÕES ESTELARES, FORMAÇÃO E EVOLUÇÃO DA GALÁXIA

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      DIAS, B et al. FORS2/VLT survey of Milky Way globular clusters: II. Fe and Mg abundances of 51 Milky Way globular clusters on a homogeneous scale. Astronomy & Astrophysics, v. 590, p. A9/1-A9/15, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201526765. Acesso em: 20 ago. 2024.
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      Dias, B., Barbuy, B. L. S., Saviane, I., Held, E. V., Da Costa, G. S., Ortolani, S., et al. (2016). FORS2/VLT survey of Milky Way globular clusters: II. Fe and Mg abundances of 51 Milky Way globular clusters on a homogeneous scale. Astronomy & Astrophysics, 590, A9/1-A9/15. doi:10.1051/0004-6361/201526765
    • NLM

      Dias B, Barbuy BLS, Saviane I, Held EV, Da Costa GS, Ortolani S, Gullieuszik M, Vásquez S. FORS2/VLT survey of Milky Way globular clusters: II. Fe and Mg abundances of 51 Milky Way globular clusters on a homogeneous scale [Internet]. Astronomy & Astrophysics. 2016 ; 590 A9/1-A9/15.[citado 2024 ago. 20 ] Available from: https://doi.org/10.1051/0004-6361/201526765
    • Vancouver

      Dias B, Barbuy BLS, Saviane I, Held EV, Da Costa GS, Ortolani S, Gullieuszik M, Vásquez S. FORS2/VLT survey of Milky Way globular clusters: II. Fe and Mg abundances of 51 Milky Way globular clusters on a homogeneous scale [Internet]. Astronomy & Astrophysics. 2016 ; 590 A9/1-A9/15.[citado 2024 ago. 20 ] Available from: https://doi.org/10.1051/0004-6361/201526765
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, CENTRO GALÁCTICO

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      BARBUY, Beatriz Leonor Silveira et al. High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP1. Astronomy & Astrophysics, v. 591, p. A53/1-A53/14, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201628106. Acesso em: 20 ago. 2024.
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      Barbuy, B. L. S., Cantelli, E., Vemado, A., Ernandes, H., Ortoloni, S., Saviane, I., et al. (2016). High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP1. Astronomy & Astrophysics, 591, A53/1-A53/14. doi:10.1051/0004-6361/201628106
    • NLM

      Barbuy BLS, Cantelli E, Vemado A, Ernandes H, Ortoloni S, Saviane I, Bica E, Minniti D, Dias B, Momany Y, Hill V, Zoccali M, Siqueira Mello C. High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP1 [Internet]. Astronomy & Astrophysics. 2016 ;591 A53/1-A53/14.[citado 2024 ago. 20 ] Available from: https://doi.org/10.1051/0004-6361/201628106
    • Vancouver

      Barbuy BLS, Cantelli E, Vemado A, Ernandes H, Ortoloni S, Saviane I, Bica E, Minniti D, Dias B, Momany Y, Hill V, Zoccali M, Siqueira Mello C. High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP1 [Internet]. Astronomy & Astrophysics. 2016 ;591 A53/1-A53/14.[citado 2024 ago. 20 ] Available from: https://doi.org/10.1051/0004-6361/201628106
  • Source: Astronomy & Astrophysics. Unidade: IAG

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

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      VAN DER SWAELMEN, M et al. Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants. Astronomy & Astrophysics, v. 586, p. A1/1-A1/11, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201525709. Acesso em: 20 ago. 2024.
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      van der Swaelmen, M., Barbuy, B. L. S., Hill, V., Zoccali, M., Minniti, D., Ortolani, S., & Gómez, A. (2016). Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants. Astronomy & Astrophysics, 586, A1/1-A1/11. doi:10.1051/0004-6361/201525709
    • NLM

      van der Swaelmen M, Barbuy BLS, Hill V, Zoccali M, Minniti D, Ortolani S, Gómez A. Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants [Internet]. Astronomy & Astrophysics. 2016 ; 586 A1/1-A1/11.[citado 2024 ago. 20 ] Available from: https://doi.org/10.1051/0004-6361/201525709
    • Vancouver

      van der Swaelmen M, Barbuy BLS, Hill V, Zoccali M, Minniti D, Ortolani S, Gómez A. Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants [Internet]. Astronomy & Astrophysics. 2016 ; 586 A1/1-A1/11.[citado 2024 ago. 20 ] Available from: https://doi.org/10.1051/0004-6361/201525709

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