Evidence for dynamically driven formation of the GW170817 neutron star binary in NGC 4993 (2017)
- Authors:
- Autor USP: LIMA, MARCOS VINICIUS BORGES TEIXEIRA - IF
- Unidade: IF
- Subjects: GALÁXIAS; COSMOLOGIA; ENERGIA ESCURA
- Language: Inglês
- Imprenta:
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ABNT
PALMESE, A. e LIMA, Marcos Vinicius Borges Teixeira. Evidence for dynamically driven formation of the GW170817 neutron star binary in NGC 4993. . São Paulo: Instituto de Física, Universidade de São Paulo. Disponível em: https://arxiv.org/abs/1710.06748. Acesso em: 19 set. 2024. , 2017 -
APA
Palmese, A., & Lima, M. V. B. T. (2017). Evidence for dynamically driven formation of the GW170817 neutron star binary in NGC 4993. São Paulo: Instituto de Física, Universidade de São Paulo. Recuperado de https://arxiv.org/abs/1710.06748 -
NLM
Palmese A, Lima MVBT. Evidence for dynamically driven formation of the GW170817 neutron star binary in NGC 4993 [Internet]. 2017 ;[citado 2024 set. 19 ] Available from: https://arxiv.org/abs/1710.06748 -
Vancouver
Palmese A, Lima MVBT. Evidence for dynamically driven formation of the GW170817 neutron star binary in NGC 4993 [Internet]. 2017 ;[citado 2024 set. 19 ] Available from: https://arxiv.org/abs/1710.06748 - A dark energy camera search for missing supergiants in the LMC after the advanced LIGO gravitational wave event GW150914
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