Spatial and temporal distributed acceleration of cosmic rays by supernova rem nants three-dimensional (1993)
- Authors:
- Autor USP: OPHER, REUVEN - IAG
- Unidade: IAG
- Assunto: ASTRONOMIA
- Language: Inglês
- Imprenta:
- Source:
- Título: Astrophysical Journal
- Volume/Número/Paginação/Ano: v.411, n.2 pt.1, p.690-707, jul. 1993
-
ABNT
MEDINA TANCO, Gustavo Adolfo e OPHER, Reuven. Spatial and temporal distributed acceleration of cosmic rays by supernova rem nants three-dimensional. Astrophysical Journal, v. 411, n. 2 pt.1, p. 690-707, 1993Tradução . . Acesso em: 10 nov. 2025. -
APA
Medina Tanco, G. A., & Opher, R. (1993). Spatial and temporal distributed acceleration of cosmic rays by supernova rem nants three-dimensional. Astrophysical Journal, 411( 2 pt.1), 690-707. -
NLM
Medina Tanco GA, Opher R. Spatial and temporal distributed acceleration of cosmic rays by supernova rem nants three-dimensional. Astrophysical Journal. 1993 ;411( 2 pt.1): 690-707.[citado 2025 nov. 10 ] -
Vancouver
Medina Tanco GA, Opher R. Spatial and temporal distributed acceleration of cosmic rays by supernova rem nants three-dimensional. Astrophysical Journal. 1993 ;411( 2 pt.1): 690-707.[citado 2025 nov. 10 ] - Where does the gravitational energy and angular momentum go in the formation of stars?
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