Chemical abundance analysis of tucana III, the second r-process enhanced ultra-faint dwarf galaxy (2018)
- Authors:
- Autor USP: LIMA, MARCOS VINICIUS BORGES TEIXEIRA - IF
- Unidade: IF
- Subjects: GALÁXIAS; COSMOLOGIA; ENERGIA ESCURA
- Language: Inglês
- Imprenta:
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ABNT
MARSHALL, J. e LIMA, Marcos Vinicius Borges Teixeira. Chemical abundance analysis of tucana III, the second r-process enhanced ultra-faint dwarf galaxy. . São Paulo: Instituto de Física, Universidade de São Paulo. Disponível em: https://arxiv.org/abs/1812.01022. Acesso em: 18 set. 2024. , 2018 -
APA
Marshall, J., & Lima, M. V. B. T. (2018). Chemical abundance analysis of tucana III, the second r-process enhanced ultra-faint dwarf galaxy. São Paulo: Instituto de Física, Universidade de São Paulo. Recuperado de https://arxiv.org/abs/1812.01022 -
NLM
Marshall J, Lima MVBT. Chemical abundance analysis of tucana III, the second r-process enhanced ultra-faint dwarf galaxy [Internet]. 2018 ;[citado 2024 set. 18 ] Available from: https://arxiv.org/abs/1812.01022 -
Vancouver
Marshall J, Lima MVBT. Chemical abundance analysis of tucana III, the second r-process enhanced ultra-faint dwarf galaxy [Internet]. 2018 ;[citado 2024 set. 18 ] Available from: https://arxiv.org/abs/1812.01022 - A dark energy camera search for missing supergiants in the LMC after the advanced LIGO gravitational wave event GW150914
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