Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis (2017)
Source: The Astrophysical Journal. Unidade: IAG
Subjects: CATÁLOGOS, GALÁXIAS, ABUNDÂNCIAS (ASTRONOMIA), GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR, POPULAÇÕES ESTELARES, ESTRELAS, CARBONO, ESPECTROSCOPIA
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BEERS, Timothy C et al. Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis. The Astrophysical Journal, v. 835, p. 81, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/835/1/81. Acesso em: 01 nov. 2024.APA
Beers, T. C., Placco, V. M., Carollo, D., Rossi, S. C. F., Lee, Y. S., Frebel, A., et al. (2017). Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis. The Astrophysical Journal, 835, 81. doi:10.3847/1538-4357/835/1/81NLM
Beers TC, Placco VM, Carollo D, Rossi SCF, Lee YS, Frebel A, Norris JE, Dietz S, Masseron T. Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis [Internet]. The Astrophysical Journal. 2017 ; 835 81.[citado 2024 nov. 01 ] Available from: https://doi.org/10.3847/1538-4357/835/1/81Vancouver
Beers TC, Placco VM, Carollo D, Rossi SCF, Lee YS, Frebel A, Norris JE, Dietz S, Masseron T. Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis [Internet]. The Astrophysical Journal. 2017 ; 835 81.[citado 2024 nov. 01 ] Available from: https://doi.org/10.3847/1538-4357/835/1/81
