Filtros : "ABUNDÂNCIA ESTELAR" "França" Removidos: "Nunes, Maria Tereza" "2018" "1917" "FFLCH" 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: 18 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. 18 ] 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. 18 ] Available from: https://doi.org/10.1051/0004-6361/201834391
  • Source: Astronomy and Astrophysysics. Unidade: IAG

    Subjects: PLANETAS, ABUNDÂNCIA ESTELAR

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    • ABNT

      MORENO, Jorge Luiz Meléndez et al. The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468. Astronomy and Astrophysysics, v. 597, p. A34, 2017Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527775. Acesso em: 18 ago. 2024.
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      Moreno, J. L. M., Bedell, M., Bean, J. L., Mello, S. F., Galarza, J. Y., Santos, L. dos, et al. (2017). The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468. Astronomy and Astrophysysics, 597, A34. doi:10.1051/0004-6361/201527775
    • NLM

      Moreno JLM, Bedell M, Bean JL, Mello SF, Galarza JY, Santos L dos, Spina L, Maia MT. The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468 [Internet]. Astronomy and Astrophysysics. 2017 ;597 A34.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201527775
    • Vancouver

      Moreno JLM, Bedell M, Bean JL, Mello SF, Galarza JY, Santos L dos, Spina L, Maia MT. The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468 [Internet]. Astronomy and Astrophysysics. 2017 ;597 A34.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201527775
  • Source: Astronomy and Astrophysysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, GALÁXIAS

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      SPITE, M et al. Abundances of the light elements from UV (HST) and red (ESO) spectra in the very old star HD 84937*. Astronomy and Astrophysysics, v. 600, p. A26, 2017Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201630058. Acesso em: 18 ago. 2024.
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      Spite, M., Peterson, R. C., Gallagher, A. J., Barbuy, B. L. S., & Spite, F. (2017). Abundances of the light elements from UV (HST) and red (ESO) spectra in the very old star HD 84937*. Astronomy and Astrophysysics, 600, A26. doi:10.1051/0004-6361/201630058
    • NLM

      Spite M, Peterson RC, Gallagher AJ, Barbuy BLS, Spite F. Abundances of the light elements from UV (HST) and red (ESO) spectra in the very old star HD 84937* [Internet]. Astronomy and Astrophysysics. 2017 ;600 A26.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201630058
    • Vancouver

      Spite M, Peterson RC, Gallagher AJ, Barbuy BLS, Spite F. Abundances of the light elements from UV (HST) and red (ESO) spectra in the very old star HD 84937* [Internet]. Astronomy and Astrophysysics. 2017 ;600 A26.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201630058
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, ABUNDÂNCIA ESTELAR

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      BENSBY, T e MORENO, Jorge Luis Meléndez. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,**. Astronomy & Astrophysics, v. 605, p. 89, 2017Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201730560. Acesso em: 18 ago. 2024.
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      Bensby, T., & Moreno, J. L. M. (2017). Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,**. Astronomy & Astrophysics, 605, 89. doi:10.1051/0004-6361/201730560
    • NLM

      Bensby T, Moreno JLM. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,** [Internet]. Astronomy & Astrophysics. 2017 ; 605 89.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201730560
    • Vancouver

      Bensby T, Moreno JLM. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,** [Internet]. Astronomy & Astrophysics. 2017 ; 605 89.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201730560
  • Source: Astronomy and Astrophysysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, GALÁXIAS

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      FRIAÇA, Amâncio César Santos e BARBUY, Beatriz Leonor Silveira. Tracing the evolution of the Galactic bulge with chemodynamical modelling of alpha-elements*. Astronomy and Astrophysysics, v. 598, p. A121, 2017Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201629941. Acesso em: 18 ago. 2024.
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      Friaça, A. C. S., & Barbuy, B. L. S. (2017). Tracing the evolution of the Galactic bulge with chemodynamical modelling of alpha-elements*. Astronomy and Astrophysysics, 598, A121. doi:10.1051/0004-6361/201629941
    • NLM

      Friaça ACS, Barbuy BLS. Tracing the evolution of the Galactic bulge with chemodynamical modelling of alpha-elements* [Internet]. Astronomy and Astrophysysics. 2017 ;598 A121.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201629941
    • Vancouver

      Friaça ACS, Barbuy BLS. Tracing the evolution of the Galactic bulge with chemodynamical modelling of alpha-elements* [Internet]. Astronomy and Astrophysysics. 2017 ;598 A121.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201629941
  • 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: 18 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. 18 ] 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. 18 ] Available from: https://doi.org/10.1051/0004-6361/201526643
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ESTRELAS, PLANETAS, GALÁXIA (VIA LÁCTEA), FORMAÇÃO E EVOLUÇÃO DA GALÁXIA

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      SPINA, Lorenzo e MORENO, Jorge Luiz Meléndez e RAMÍREZ, Iván. Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars. Astronomy & Astrophysics, v. 585, p. A152/1-A152/15, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527429. Acesso em: 18 ago. 2024.
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      Spina, L., Moreno, J. L. M., & Ramírez, I. (2016). Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars. Astronomy & Astrophysics, 585, A152/1-A152/15. doi:10.1051/0004-6361/201527429
    • NLM

      Spina L, Moreno JLM, Ramírez I. Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars [Internet]. Astronomy & Astrophysics. 2016 ; 585 A152/1-A152/15.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201527429
    • Vancouver

      Spina L, Moreno JLM, Ramírez I. Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars [Internet]. Astronomy & Astrophysics. 2016 ; 585 A152/1-A152/15.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201527429
  • Source: Astronomy & Astrophysics. Unidade: IAG

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

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      REGGIANI, Henrique et al. First high-precision differential abundance analysis of extremely metal-poor stars. Astronomy & Astrophysics, v. 586, p. A67/1-A67/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527439. Acesso em: 18 ago. 2024.
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      Reggiani, H., Moreno, J. L. M., Yong, D., Ramírez, I., & Asplund, M. (2016). First high-precision differential abundance analysis of extremely metal-poor stars. Astronomy & Astrophysics, 586, A67/1-A67/8. doi:10.1051/0004-6361/201527439
    • NLM

      Reggiani H, Moreno JLM, Yong D, Ramírez I, Asplund M. First high-precision differential abundance analysis of extremely metal-poor stars [Internet]. Astronomy & Astrophysics. 2016 ; 586 A67/1-A67/8.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201527439
    • Vancouver

      Reggiani H, Moreno JLM, Yong D, Ramírez I, Asplund M. First high-precision differential abundance analysis of extremely metal-poor stars [Internet]. Astronomy & Astrophysics. 2016 ; 586 A67/1-A67/8.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201527439
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIAS SOLARES, ABUNDÂNCIA ESTELAR, TERRA (PLANETA), PLANETAS

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      GALARZA, Jhon Yana e MORENO, Jorge Luiz Meléndez e COHEN, Judith G. Serendipitous discovery of the faint solar twin Inti 1. Astronomy & Astrophysics, v. 589, p. A65/1-A65/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527477. Acesso em: 18 ago. 2024.
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      Galarza, J. Y., Moreno, J. L. M., & Cohen, J. G. (2016). Serendipitous discovery of the faint solar twin Inti 1. Astronomy & Astrophysics, 589, A65/1-A65/8. doi:10.1051/0004-6361/201527477
    • NLM

      Galarza JY, Moreno JLM, Cohen JG. Serendipitous discovery of the faint solar twin Inti 1 [Internet]. Astronomy & Astrophysics. 2016 ; 589 A65/1-A65/8.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201527477
    • Vancouver

      Galarza JY, Moreno JLM, Cohen JG. Serendipitous discovery of the faint solar twin Inti 1 [Internet]. Astronomy & Astrophysics. 2016 ; 589 A65/1-A65/8.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201527477
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ABUNDÂNCIAS (ASTRONOMIA), ESTRELAS, 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. 588, p. A66, 2016Tradução . . Disponível em: https://arxiv.org/pdf/1602.00058.pdf. Acesso em: 18 ago. 2024.
    • APA

      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, 588, A66. 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 ; 588 A66.[citado 2024 ago. 18 ] Available from: https://arxiv.org/pdf/1602.00058.pdf
    • 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 ; 588 A66.[citado 2024 ago. 18 ] Available from: https://arxiv.org/pdf/1602.00058.pdf
  • 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: 18 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. 18 ] 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. 18 ] Available from: https://doi.org/10.1051/0004-6361/201526765
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIAS SOLARES, ABUNDÂNCIA ESTELAR, PLANETAS

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      GALARZA, Jhon Yana et al. High-precision analysis of the solar twin HIP 100963. Astronomy & Astrophysics, v. 589, p. A17/1-A17/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527912. Acesso em: 18 ago. 2024.
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      Galarza, J. Y., Moreno, J. L. M., Ramírez, I., Yong, D., Karakas, A. I., Asplund, M., & Liu, F. (2016). High-precision analysis of the solar twin HIP 100963. Astronomy & Astrophysics, 589, A17/1-A17/8. doi:10.1051/0004-6361/201527912
    • NLM

      Galarza JY, Moreno JLM, Ramírez I, Yong D, Karakas AI, Asplund M, Liu F. High-precision analysis of the solar twin HIP 100963 [Internet]. Astronomy & Astrophysics. 2016 ; 589 A17/1-A17/8.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201527912
    • Vancouver

      Galarza JY, Moreno JLM, Ramírez I, Yong D, Karakas AI, Asplund M, Liu F. High-precision analysis of the solar twin HIP 100963 [Internet]. Astronomy & Astrophysics. 2016 ; 589 A17/1-A17/8.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201527912
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Assunto: ABUNDÂNCIA ESTELAR

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      MORENO, Jorge Luiz Meléndez et al. 2 MASS J18082002-5104378: The brightest (V = 11.9) ultra metal-poor star. Astronomy & Astrophysics, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527456. Acesso em: 18 ago. 2024.
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      Moreno, J. L. M., Placco, V. M., Tucci-Maia, M., Ramírez, I., Li, T. S., & Perez, G. (2016). 2 MASS J18082002-5104378: The brightest (V = 11.9) ultra metal-poor star. Astronomy & Astrophysics. doi:10.1051/0004-6361/201527456
    • NLM

      Moreno JLM, Placco VM, Tucci-Maia M, Ramírez I, Li TS, Perez G. 2 MASS J18082002-5104378: The brightest (V = 11.9) ultra metal-poor star [Internet]. Astronomy & Astrophysics. 2016 ;[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201527456
    • Vancouver

      Moreno JLM, Placco VM, Tucci-Maia M, Ramírez I, Li TS, Perez G. 2 MASS J18082002-5104378: The brightest (V = 11.9) ultra metal-poor star [Internet]. Astronomy & Astrophysics. 2016 ;[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201527456
  • 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: 18 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. 18 ] 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. 18 ] 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: 18 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. 18 ] 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. 18 ] Available from: https://doi.org/10.1051/0004-6361/201525709
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, POPULAÇÕES ESTELARES, ESTRELAS

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      MORENO, Jorge Luiz Meléndez et al. 2MASS J18082002-5104378: the brightest (V=11.9) ultra-metal poor star. Astronomy & Astrophysics, v. 585, p. L5/1-L5/5, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527456. Acesso em: 18 ago. 2024.
    • APA

      Moreno, J. L. M., Placco, V. M., Tucci-Maia, M., Ramírez, I., Li, T. S., & Perez, G. (2016). 2MASS J18082002-5104378: the brightest (V=11.9) ultra-metal poor star. Astronomy & Astrophysics, 585, L5/1-L5/5. doi:10.1051/0004-6361/201527456
    • NLM

      Moreno JLM, Placco VM, Tucci-Maia M, Ramírez I, Li TS, Perez G. 2MASS J18082002-5104378: the brightest (V=11.9) ultra-metal poor star [Internet]. Astronomy & Astrophysics. 2016 ; 585 L5/1-L5/5.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201527456
    • Vancouver

      Moreno JLM, Placco VM, Tucci-Maia M, Ramírez I, Li TS, Perez G. 2MASS J18082002-5104378: the brightest (V=11.9) ultra-metal poor star [Internet]. Astronomy & Astrophysics. 2016 ; 585 L5/1-L5/5.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201527456
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: CENTRO GALÁCTICO, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES

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      SIQUEIRA-MELLO, C et al. Looking for imprints of the first stellar generations in metal-poor bulge field stars. Astronomy & Astrophysics, v. 593, p. A79/1-A79/16, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201628104. Acesso em: 18 ago. 2024.
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      Siqueira-Mello, C., Chiappini, C., Barbuy, B. L. S., & Cantelli, E. (2016). Looking for imprints of the first stellar generations in metal-poor bulge field stars. Astronomy & Astrophysics, 593, A79/1-A79/16. doi:10.1051/0004-6361/201628104
    • NLM

      Siqueira-Mello C, Chiappini C, Barbuy BLS, Cantelli E. Looking for imprints of the first stellar generations in metal-poor bulge field stars [Internet]. Astronomy & Astrophysics. 2016 ; 593 A79/1-A79/16.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201628104
    • Vancouver

      Siqueira-Mello C, Chiappini C, Barbuy BLS, Cantelli E. Looking for imprints of the first stellar generations in metal-poor bulge field stars [Internet]. Astronomy & Astrophysics. 2016 ; 593 A79/1-A79/16.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201628104
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, GALÁXIAS ELÍPTICAS

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      WALCHER, C. J et al. Self-similarity in the chemical evolution of galaxies and the delay-time distribution of SNe Ia. Astronomy and Astrophysics, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201528019. Acesso em: 18 ago. 2024.
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      Walcher, C. J., Yates, R. M., Minchev, I., & Coelho, P. R. T. (2016). Self-similarity in the chemical evolution of galaxies and the delay-time distribution of SNe Ia. Astronomy and Astrophysics. doi:10.1051/0004-6361/201528019
    • NLM

      Walcher CJ, Yates RM, Minchev I, Coelho PRT. Self-similarity in the chemical evolution of galaxies and the delay-time distribution of SNe Ia [Internet]. Astronomy and Astrophysics. 2016 ;[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201528019
    • Vancouver

      Walcher CJ, Yates RM, Minchev I, Coelho PRT. Self-similarity in the chemical evolution of galaxies and the delay-time distribution of SNe Ia [Internet]. Astronomy and Astrophysics. 2016 ;[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201528019
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, EVOLUÇÃO ESTELAR, FORMAÇÃO E EVOLUÇÃO DA GALÁXIA

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      TUCCI MAIA, M et al. The Solar Twin Planet Search: III. The [Y/Mg] clock: estimating stellar ages of solar-type stars. Astronomy & Astrophysics, v. 590, p. A32/1-A32/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527848. Acesso em: 18 ago. 2024.
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      Tucci Maia, M., Ramírez, I., Moreno, J. L. M., Bedell, M., Bean, J. L., & Asplund, M. (2016). The Solar Twin Planet Search: III. The [Y/Mg] clock: estimating stellar ages of solar-type stars. Astronomy & Astrophysics, 590, A32/1-A32/8. doi:10.1051/0004-6361/201527848
    • NLM

      Tucci Maia M, Ramírez I, Moreno JLM, Bedell M, Bean JL, Asplund M. The Solar Twin Planet Search: III. The [Y/Mg] clock: estimating stellar ages of solar-type stars [Internet]. Astronomy & Astrophysics. 2016 ; 590 A32/1-A32/8.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201527848
    • Vancouver

      Tucci Maia M, Ramírez I, Moreno JLM, Bedell M, Bean JL, Asplund M. The Solar Twin Planet Search: III. The [Y/Mg] clock: estimating stellar ages of solar-type stars [Internet]. Astronomy & Astrophysics. 2016 ; 590 A32/1-A32/8.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201527848
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, EVOLUÇÃO ESTELAR, PLANETAS

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      CARLOS, Marília e NISSEN, Poul E e MORENO, Jorge Luiz Meléndez. Correlation between lithium abundances and ages of solar twin stars. Astronomy & Astrophysics, v. 587, p. A100/1-A100/6, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527478. Acesso em: 18 ago. 2024.
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      Carlos, M., Nissen, P. E., & Moreno, J. L. M. (2016). Correlation between lithium abundances and ages of solar twin stars. Astronomy & Astrophysics, 587, A100/1-A100/6. doi:10.1051/0004-6361/201527478
    • NLM

      Carlos M, Nissen PE, Moreno JLM. Correlation between lithium abundances and ages of solar twin stars [Internet]. Astronomy & Astrophysics. 2016 ; 587 A100/1-A100/6.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201527478
    • Vancouver

      Carlos M, Nissen PE, Moreno JLM. Correlation between lithium abundances and ages of solar twin stars [Internet]. Astronomy & Astrophysics. 2016 ; 587 A100/1-A100/6.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1051/0004-6361/201527478

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