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

    Subjects: ESTRELAS BINÁRIAS, TRANSFERÊNCIA RADIATIVA

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      SUFFAK, M W et al. Non-LTE Monte Carlo radiative transfer.: III. the thermal properties of tilted and warped be star discs. Monthly Notices of the Royal Astronomical Society, 2023Tradução . . Disponível em: https://doi.org/10.1093/mnras/stad2781. Acesso em: 15 abr. 2024.
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      Suffak, M. W., Jones, C. E., Carciofi, A. C., & Amorim, T. H. (2023). Non-LTE Monte Carlo radiative transfer.: III. the thermal properties of tilted and warped be star discs. Monthly Notices of the Royal Astronomical Society. doi:10.1093/mnras/stad2781
    • NLM

      Suffak MW, Jones CE, Carciofi AC, Amorim TH. Non-LTE Monte Carlo radiative transfer.: III. the thermal properties of tilted and warped be star discs [Internet]. Monthly Notices of the Royal Astronomical Society. 2023 ;[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/stad2781
    • Vancouver

      Suffak MW, Jones CE, Carciofi AC, Amorim TH. Non-LTE Monte Carlo radiative transfer.: III. the thermal properties of tilted and warped be star discs [Internet]. Monthly Notices of the Royal Astronomical Society. 2023 ;[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/stad2781
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Assunto: ESTRELAS BINÁRIAS

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      RUBIO, A. C et al. Bayesian sampling with BeAtlas, a grid of synthetic Be star spectra: I. Recovering the fundamental parameters of 𝛼 Eri and 𝛽 CMi. Monthly Notices of the Royal Astronomical Society, 2023Tradução . . Disponível em: https://doi.org/10.1093/mnras/stad2652. Acesso em: 15 abr. 2024.
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      Rubio, A. C., Carciofi, A. C., Ticiani, P., Mota, B. C., Amorim, T. H., & Silva, A. C. F. (2023). Bayesian sampling with BeAtlas, a grid of synthetic Be star spectra: I. Recovering the fundamental parameters of 𝛼 Eri and 𝛽 CMi. Monthly Notices of the Royal Astronomical Society. doi:10.1093/mnras/stad2652
    • NLM

      Rubio AC, Carciofi AC, Ticiani P, Mota BC, Amorim TH, Silva ACF. Bayesian sampling with BeAtlas, a grid of synthetic Be star spectra: I. Recovering the fundamental parameters of 𝛼 Eri and 𝛽 CMi [Internet]. Monthly Notices of the Royal Astronomical Society. 2023 ;[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/stad2652
    • Vancouver

      Rubio AC, Carciofi AC, Ticiani P, Mota BC, Amorim TH, Silva ACF. Bayesian sampling with BeAtlas, a grid of synthetic Be star spectra: I. Recovering the fundamental parameters of 𝛼 Eri and 𝛽 CMi [Internet]. Monthly Notices of the Royal Astronomical Society. 2023 ;[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/stad2652
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: HIDRODINÂMICA, CAMPO MAGNÉTICO, ESTRELAS, POLARIZAÇÃO (ASTRONOMIA)

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      MUNOZ, M S et al. Untangling magnetic massive star properties with linear polarization variability and the analytic dynamical magnetosphere model. Monthly Notices of the Royal Astronomical Society, v. 511, p. 3228-3249, 2022Tradução . . Disponível em: https://doi.org/10.1093/mnras/stab3767. Acesso em: 15 abr. 2024.
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      Munoz, M. S., Wade G A,, Faes, D. M., Carciofi, A. C., & Labadie-Bartz, J. (2022). Untangling magnetic massive star properties with linear polarization variability and the analytic dynamical magnetosphere model. Monthly Notices of the Royal Astronomical Society, 511, 3228-3249. doi:10.1093/mnras/stab3767
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      Munoz MS, Wade G A, Faes DM, Carciofi AC, Labadie-Bartz J. Untangling magnetic massive star properties with linear polarization variability and the analytic dynamical magnetosphere model [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 511 3228-3249.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/stab3767
    • Vancouver

      Munoz MS, Wade G A, Faes DM, Carciofi AC, Labadie-Bartz J. Untangling magnetic massive star properties with linear polarization variability and the analytic dynamical magnetosphere model [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 511 3228-3249.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/stab3767
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ESTRELAS BINÁRIAS, ASTROFÍSICA ESTELAR

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      SUFFAK, M e JONES, C E e CARCIOFI, Alex Cavaliéri. Growth and dissipation of Be star discs in misaligned binary systems. Monthly Notices of the Royal Astronomical Society, v. 509, p. 931-944, 2022Tradução . . Disponível em: https://doi.org/10.1093/mnras/stab3024. Acesso em: 15 abr. 2024.
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      Suffak, M., Jones, C. E., & Carciofi, A. C. (2022). Growth and dissipation of Be star discs in misaligned binary systems. Monthly Notices of the Royal Astronomical Society, 509, 931-944. doi:10.1093/mnras/stab3024
    • NLM

      Suffak M, Jones CE, Carciofi AC. Growth and dissipation of Be star discs in misaligned binary systems [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ;509 931-944.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/stab3024
    • Vancouver

      Suffak M, Jones CE, Carciofi AC. Growth and dissipation of Be star discs in misaligned binary systems [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ;509 931-944.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/stab3024
  • Source: Monthly Notices of the Royal Astronomical Society. Unidades: IAG, IF

    Subjects: ATMOSFERAS ESTELARES, ABUNDÂNCIA ESTELAR, ESTRELAS

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      RAZERA, R et al. Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid. Monthly Notices of the Royal Astronomical Society, v. 517, p. 4590-4606, 2022Tradução . . Disponível em: https://academic.oup.com/mnras/article/517/3/4590/6653110. Acesso em: 15 abr. 2024.
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      Razera, R., Barbuy, B. L. S., Moura, T. C., Ernandes, H., & Friaça, A. C. S. (2022). Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid. Monthly Notices of the Royal Astronomical Society, 517, 4590-4606. doi:10.1093/mnras/stac2136
    • NLM

      Razera R, Barbuy BLS, Moura TC, Ernandes H, Friaça ACS. Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 517 4590-4606.[citado 2024 abr. 15 ] Available from: https://academic.oup.com/mnras/article/517/3/4590/6653110
    • Vancouver

      Razera R, Barbuy BLS, Moura TC, Ernandes H, Friaça ACS. Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 517 4590-4606.[citado 2024 abr. 15 ] Available from: https://academic.oup.com/mnras/article/517/3/4590/6653110
  • Source: Monthly Notices of the Royal Astronomical Society. Unidades: IF, IAG

    Assunto: ESTRELAS

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      YUAN, H-B et al. The miniJPAS survey: stellar atmospheric parameters from 56 optical filters. Monthly Notices of the Royal Astronomical Society, v. 518, n. 2, p. 2018–2033, 2022Tradução . . Disponível em: https://doi.org/10.1093/mnras/stac3155. Acesso em: 15 abr. 2024.
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      Yuan, H. -B., Abramo, L. R. W., Oliveira, C. L. M. de, & Sodré Júnior, L. (2022). The miniJPAS survey: stellar atmospheric parameters from 56 optical filters. Monthly Notices of the Royal Astronomical Society, 518( 2), 2018–2033. doi:10.1093/mnras/stac3155
    • NLM

      Yuan H-B, Abramo LRW, Oliveira CLM de, Sodré Júnior L. The miniJPAS survey: stellar atmospheric parameters from 56 optical filters [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 518( 2): 2018–2033.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/stac3155
    • Vancouver

      Yuan H-B, Abramo LRW, Oliveira CLM de, Sodré Júnior L. The miniJPAS survey: stellar atmospheric parameters from 56 optical filters [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 518( 2): 2018–2033.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/stac3155
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: 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: 15 abr. 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
    • NLM

      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 abr. 15 ] 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 abr. 15 ] Available from: https://doi.org/10.1093/mnras/stab3789
  • Source: Monthly Notices of the Royal Astronomical Society. Unidades: IAG, EACH

    Subjects: EFEITOS ATMOSFÉRICOS, ESTRELAS BINÁRIAS, ETA CARINAE, PERDA DE MASSA

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      ABRAHAM, Zulema et al. Telluric absorption lines in the ALMA spectra of η Car. Monthly Notices of the Royal Astronomical Society, v. No 2022, p. 47-58, 2022Tradução . . Disponível em: https://doi.org/10.1093/mnras/stac2661. Acesso em: 15 abr. 2024.
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      Abraham, Z., Beaklini, P. P. B., Cox, P., Gonçalves, D. A. F., & Nyman, L. -Å. (2022). Telluric absorption lines in the ALMA spectra of η Car. Monthly Notices of the Royal Astronomical Society, No 2022, 47-58. doi:10.1093/mnras/stac2661
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      Abraham Z, Beaklini PPB, Cox P, Gonçalves DAF, Nyman L-Å. Telluric absorption lines in the ALMA spectra of η Car [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; No 2022 47-58.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/stac2661
    • Vancouver

      Abraham Z, Beaklini PPB, Cox P, Gonçalves DAF, Nyman L-Å. Telluric absorption lines in the ALMA spectra of η Car [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; No 2022 47-58.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/stac2661
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Assunto: CAMPO MAGNÉTICO

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      SANTOS-LIMA, R et al. Diffusion of large-scale magnetic fields by reconnection in MHD turbulence. Monthly Notices of the Royal Astronomical Society, v. 503, p. 1290-1309, 2021Tradução . . Disponível em: https://academic.oup.com/mnras/article/503/1/1290/6144594. Acesso em: 15 abr. 2024.
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      Santos-Lima, R., Guerrero, G., Dal Pino, E. M. de G., & Lazarian, A. (2021). Diffusion of large-scale magnetic fields by reconnection in MHD turbulence. Monthly Notices of the Royal Astronomical Society, 503, 1290-1309. doi:10.1093/mnras/stab470
    • NLM

      Santos-Lima R, Guerrero G, Dal Pino EM de G, Lazarian A. Diffusion of large-scale magnetic fields by reconnection in MHD turbulence [Internet]. Monthly Notices of the Royal Astronomical Society. 2021 ; 503 1290-1309.[citado 2024 abr. 15 ] Available from: https://academic.oup.com/mnras/article/503/1/1290/6144594
    • Vancouver

      Santos-Lima R, Guerrero G, Dal Pino EM de G, Lazarian A. Diffusion of large-scale magnetic fields by reconnection in MHD turbulence [Internet]. Monthly Notices of the Royal Astronomical Society. 2021 ; 503 1290-1309.[citado 2024 abr. 15 ] Available from: https://academic.oup.com/mnras/article/503/1/1290/6144594
  • Source: Monthly Notices of the Royal Astronomical Society. Unidades: IAG, IME, IF

    Subjects: AGLOMERADOS DE GALÁXIAS, QUASARES, APRENDIZADO COMPUTACIONAL

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      NAKAZONO, Lilianne Mariko Izuti et al. On the discovery of stars, quasars, and galaxies in the Southern Hemisphere with S-PLUS DR2. Monthly Notices of the Royal Astronomical Society, v. 507, n. 4, p. 5847-5868, 2021Tradução . . Disponível em: https://doi.org/10.1093/mnras/stab1835. Acesso em: 15 abr. 2024.
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      Nakazono, L. M. I., Oliveira, C. M. de, Hirata, N. S. T., Jeram, S., Queiroz, C., Eikenberry, S., et al. (2021). On the discovery of stars, quasars, and galaxies in the Southern Hemisphere with S-PLUS DR2. Monthly Notices of the Royal Astronomical Society, 507( 4), 5847-5868. doi:10.1093/mnras/stab1835
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      Nakazono LMI, Oliveira CM de, Hirata NST, Jeram S, Queiroz C, Eikenberry S, Gonzalez AH, Abramo LRW, Overzier R, Espadoto M, Martinazzo ACRC, Sampedro L, Herpich FR, Fernandes F de A, Werle A, Barbosa CE, Sodre Junior L, Lima EV, Buzzo MLG, Cortesi A, Menendez-Delmestre K, Akras S, Alvarez-Candal A, Lopes AR, Telles E, Schoenell W, Kanaan A, Ribeiro T. On the discovery of stars, quasars, and galaxies in the Southern Hemisphere with S-PLUS DR2 [Internet]. Monthly Notices of the Royal Astronomical Society. 2021 ; 507( 4): 5847-5868.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/stab1835
    • Vancouver

      Nakazono LMI, Oliveira CM de, Hirata NST, Jeram S, Queiroz C, Eikenberry S, Gonzalez AH, Abramo LRW, Overzier R, Espadoto M, Martinazzo ACRC, Sampedro L, Herpich FR, Fernandes F de A, Werle A, Barbosa CE, Sodre Junior L, Lima EV, Buzzo MLG, Cortesi A, Menendez-Delmestre K, Akras S, Alvarez-Candal A, Lopes AR, Telles E, Schoenell W, Kanaan A, Ribeiro T. On the discovery of stars, quasars, and galaxies in the Southern Hemisphere with S-PLUS DR2 [Internet]. Monthly Notices of the Royal Astronomical Society. 2021 ; 507( 4): 5847-5868.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/stab1835
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ESTRELAS BINÁRIAS, ECLIPSE

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      ALMEIDA, L. A. L. de et al. Eclipse timing variation of GK Vir: evidence of a possible Jupiter-like planet in a circumbinary orbit. Monthly Notices of the Royal Astronomical Society, v. 497, p. 4022-4029, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/staa2185. Acesso em: 15 abr. 2024.
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      Almeida, L. A. L. de, Pereira, E. S., Sterken, C., Pigulski, A., Koenigsberger, G., Moffat, A. F. J., et al. (2020). Eclipse timing variation of GK Vir: evidence of a possible Jupiter-like planet in a circumbinary orbit. Monthly Notices of the Royal Astronomical Society, 497, 4022-4029. doi:10.1093/mnras/staa2185
    • NLM

      Almeida LAL de, Pereira ES, Sterken C, Pigulski A, Koenigsberger G, Moffat AFJ, Madura TI, Hamaguichi K, Corcoran MF, Damineli Neto A. Eclipse timing variation of GK Vir: evidence of a possible Jupiter-like planet in a circumbinary orbit [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 497 4022-4029.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/staa2185
    • Vancouver

      Almeida LAL de, Pereira ES, Sterken C, Pigulski A, Koenigsberger G, Moffat AFJ, Madura TI, Hamaguichi K, Corcoran MF, Damineli Neto A. Eclipse timing variation of GK Vir: evidence of a possible Jupiter-like planet in a circumbinary orbit [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 497 4022-4029.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/staa2185
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: 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: 15 abr. 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
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      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 abr. 15 ] 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 abr. 15 ] Available from: https://doi.org/10.1093/mnras/staa3051
  • Source: Monthly Notices of the Royal Astronomical Society. Unidades: IAG, IF

    Subjects: ASTROFÍSICA, UNIVERSO PRIMORDIAL, COSMOLOGIA, QUASARES, ESTRUTURA DO UNIVERSO, GALÁXIAS

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      CARVALHO, E. de et al. Baryon acoustic oscillations signature in the three-point angular correlation function from the SDSS-DR12 quasar survey. Monthly Notices of the Royal Astronomical Society, v. 492, n. 3, p. 4469-4476, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/staa119. Acesso em: 15 abr. 2024.
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      Carvalho, E. de, Bernui, A., Xavier, H. S., & Novaes, C. P. (2020). Baryon acoustic oscillations signature in the three-point angular correlation function from the SDSS-DR12 quasar survey. Monthly Notices of the Royal Astronomical Society, 492( 3), 4469-4476. doi:10.1093/mnras/staa119
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      Carvalho E de, Bernui A, Xavier HS, Novaes CP. Baryon acoustic oscillations signature in the three-point angular correlation function from the SDSS-DR12 quasar survey [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 492( 3): 4469-4476.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/staa119
    • Vancouver

      Carvalho E de, Bernui A, Xavier HS, Novaes CP. Baryon acoustic oscillations signature in the three-point angular correlation function from the SDSS-DR12 quasar survey [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 492( 3): 4469-4476.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/staa119
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDANCIA ESTELAR, FORMAÇÃO DE ESTRELAS

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      BOTELHO, R. B. et al. Carbon, isotopic ratio C-12/C-13, and nitrogen in solar twins: constraints for the chemical evolution of the local disc. Monthly Notices of the Royal Astronomical Society, v. 499, p. 2196-2213, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/staa2917. Acesso em: 15 abr. 2024.
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      Botelho, R. B., Milone, A. de C., Moreno, J. L. M., Alves-Brito, A., Spina, L., & Bean, J. L. (2020). Carbon, isotopic ratio C-12/C-13, and nitrogen in solar twins: constraints for the chemical evolution of the local disc. Monthly Notices of the Royal Astronomical Society, 499, 2196-2213. doi:10.1093/mnras/staa2917
    • NLM

      Botelho RB, Milone A de C, Moreno JLM, Alves-Brito A, Spina L, Bean JL. Carbon, isotopic ratio C-12/C-13, and nitrogen in solar twins: constraints for the chemical evolution of the local disc [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 499 2196-2213.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/staa2917
    • Vancouver

      Botelho RB, Milone A de C, Moreno JLM, Alves-Brito A, Spina L, Bean JL. Carbon, isotopic ratio C-12/C-13, and nitrogen in solar twins: constraints for the chemical evolution of the local disc [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 499 2196-2213.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/staa2917
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: MATÉRIA ESCURA, COSMOLOGIA, ESTRUTURA DO UNIVERSO

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      ABRIL, Javier et al. Disentangling cataclysmic variables in Gaia's HR diagram. Monthly Notices of the Royal Astronomical Society, v. 492, n. 1, p. L78–88, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnrasl/slz181. Acesso em: 15 abr. 2024.
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      abril, J., Schmidtobreick, L., Ederoclite, A., & López-Sanjuan, C. (2020). Disentangling cataclysmic variables in Gaia's HR diagram. Monthly Notices of the Royal Astronomical Society, 492( 1), L78–88. doi:10.1093/mnrasl/slz181
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      abril J, Schmidtobreick L, Ederoclite A, López-Sanjuan C. Disentangling cataclysmic variables in Gaia's HR diagram [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 492( 1): L78–88.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnrasl/slz181
    • Vancouver

      abril J, Schmidtobreick L, Ederoclite A, López-Sanjuan C. Disentangling cataclysmic variables in Gaia's HR diagram [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 492( 1): L78–88.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnrasl/slz181
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ESTRELAS BINÁRIAS, ASTROFÍSICA ESTELAR

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      ISABELLE , H Cyr e CARCIOFI, Alex Cavaliéri e OKAZAKI, A T. Spiral density enhancements in Be binary systems. Monthly Notices of the Royal Astronomical Society, v. 497, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/staa2176. Acesso em: 15 abr. 2024.
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      Isabelle , H. C., Carciofi, A. C., & Okazaki, A. T. (2020). Spiral density enhancements in Be binary systems. Monthly Notices of the Royal Astronomical Society, 497. doi:10.1093/mnras/staa2176
    • NLM

      Isabelle HC, Carciofi AC, Okazaki AT. Spiral density enhancements in Be binary systems [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ;497[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/staa2176
    • Vancouver

      Isabelle HC, Carciofi AC, Okazaki AT. Spiral density enhancements in Be binary systems [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ;497[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/staa2176
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: GALÁXIAS ELÍPTICAS, COSMOLOGIA, GALÁXIAS

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      WERLE, A et al. Clues on the history of early-type galaxies from SDSS spectra and GALEX photometry. Monthly Notices of the Royal Astronomical Society, v. 497, p. 3251-3263, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/staa2217. Acesso em: 15 abr. 2024.
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      Werle, A., Fernandes, R. C., Asari, N. V., Coelho, P. R. T., Carvalho, R. R. de, Herpich, F. R., et al. (2020). Clues on the history of early-type galaxies from SDSS spectra and GALEX photometry. Monthly Notices of the Royal Astronomical Society, 497, 3251-3263. doi:10.1093/mnras/staa2217
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      Werle A, Fernandes RC, Asari NV, Coelho PRT, Carvalho RR de, Herpich FR, Oliveira CLM de, Sodré Júnior L, Ruschel-Dutra D, Amorin A de, Sampaio VM. Clues on the history of early-type galaxies from SDSS spectra and GALEX photometry [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 497 3251-3263.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/staa2217
    • Vancouver

      Werle A, Fernandes RC, Asari NV, Coelho PRT, Carvalho RR de, Herpich FR, Oliveira CLM de, Sodré Júnior L, Ruschel-Dutra D, Amorin A de, Sampaio VM. Clues on the history of early-type galaxies from SDSS spectra and GALEX photometry [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 497 3251-3263.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/staa2217
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: GALÁXIAS, GALÁXIAS ELÍPTICAS

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      DANTAS, M. L. L e COELHO, Paula Rodrigues Teixeira e GONÇALVES, T S. UV bright red-sequence galaxies: how do UV upturn systems evolve in redshift and stellar mass?. Monthly Notices of the Royal Astronomical Society, v. 492, n. 2, p. 2996-3011, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz3609. Acesso em: 15 abr. 2024.
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      Dantas, M. L. L., Coelho, P. R. T., & Gonçalves, T. S. (2020). UV bright red-sequence galaxies: how do UV upturn systems evolve in redshift and stellar mass? Monthly Notices of the Royal Astronomical Society, 492( 2), 2996-3011. doi:10.1093/mnras/stz3609
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      Dantas MLL, Coelho PRT, Gonçalves TS. UV bright red-sequence galaxies: how do UV upturn systems evolve in redshift and stellar mass? [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 492( 2): 2996-3011.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/stz3609
    • Vancouver

      Dantas MLL, Coelho PRT, Gonçalves TS. UV bright red-sequence galaxies: how do UV upturn systems evolve in redshift and stellar mass? [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 492( 2): 2996-3011.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/stz3609
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: GALÁXIAS, NUVENS DE MAGALHÃES, FOTOMETRIA

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      SANTOS JÚNIOR, João F. C. et al. The VISCACHA survey – II. Structure of star clusters in the Magellanic Clouds periphery. Monthly Notices of the Royal Astronomical Society, v. 498, p. 205-222, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/staa2425. Acesso em: 15 abr. 2024.
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      Santos Júnior, J. F. C., Maia, F. F. S., Pérez-Villegas, A., Dias, B., Kerber, L. de O., & Barbuy, B. L. S. (2020). The VISCACHA survey – II. Structure of star clusters in the Magellanic Clouds periphery. Monthly Notices of the Royal Astronomical Society, 498, 205-222. doi:10.1093/mnras/staa2425
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      Santos Júnior JFC, Maia FFS, Pérez-Villegas A, Dias B, Kerber L de O, Barbuy BLS. The VISCACHA survey – II. Structure of star clusters in the Magellanic Clouds periphery [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 498 205-222.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/staa2425
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      Santos Júnior JFC, Maia FFS, Pérez-Villegas A, Dias B, Kerber L de O, Barbuy BLS. The VISCACHA survey – II. Structure of star clusters in the Magellanic Clouds periphery [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 498 205-222.[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/staa2425
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ASTROMETRIA, FORMAÇÃO DE ESTRELAS

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      LORENZO-GUTIÉRREZ, A. e EDEROCLITE, Alessandro. Deriving stellar parameters from GALANTE photometry: bias and precision. Monthly Notices of the Royal Astronomical Society, v. 494, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/staa892. Acesso em: 15 abr. 2024.
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      Lorenzo-Gutiérrez, A., & Ederoclite, A. (2020). Deriving stellar parameters from GALANTE photometry: bias and precision. Monthly Notices of the Royal Astronomical Society, 494. doi:10.1093/mnras/staa892
    • NLM

      Lorenzo-Gutiérrez A, Ederoclite A. Deriving stellar parameters from GALANTE photometry: bias and precision [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 494[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/staa892
    • Vancouver

      Lorenzo-Gutiérrez A, Ederoclite A. Deriving stellar parameters from GALANTE photometry: bias and precision [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 494[citado 2024 abr. 15 ] Available from: https://doi.org/10.1093/mnras/staa892

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