Crust Composition and the Shallow Heat Source in KS 1731–260 (2025)
Source: Physical Review Letters. Unidade: IF
Subjects: FÍSICA NUCLEAR, ESTRELAS DE NEUTRONS, ASTROFÍSICA, NÊUTRONS
ABNT
JAIN, R. et al. Crust Composition and the Shallow Heat Source in KS 1731–260. Physical Review Letters, 2025Tradução . . Disponível em: https://doi.org/10.1103/jwc8-xfhv. Acesso em: 04 jan. 2026.APA
Jain, R., Brown, E. F., Schatz, H., Afanasjev, A. V., Beard, M., Gasques, L. R., et al. (2025). Crust Composition and the Shallow Heat Source in KS 1731–260. Physical Review Letters. doi:https://doi.org/10.1103/jwc8-xfhvNLM
Jain R, Brown EF, Schatz H, Afanasjev AV, Beard M, Gasques LR, Grace J, Heger A, Hitt GW, Hix WR, Lau R, Ong W-J, Wiescher M, Xu Y. Crust Composition and the Shallow Heat Source in KS 1731–260 [Internet]. Physical Review Letters. 2025 ;[citado 2026 jan. 04 ] Available from: https://doi.org/10.1103/jwc8-xfhvVancouver
Jain R, Brown EF, Schatz H, Afanasjev AV, Beard M, Gasques LR, Grace J, Heger A, Hitt GW, Hix WR, Lau R, Ong W-J, Wiescher M, Xu Y. Crust Composition and the Shallow Heat Source in KS 1731–260 [Internet]. Physical Review Letters. 2025 ;[citado 2026 jan. 04 ] Available from: https://doi.org/10.1103/jwc8-xfhv
