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: 14 maio 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 maio 14 ] -
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 maio 14 ] - Can black holes provide the energy for active galactic nuclei, quasars, and gamma ray bursts?
- On the thickness of a mildly relativistic collisional shock wave
- A new method for studying the topology ofthe universefrom cosmic microwave background data
- Origem de campos magnéticos primordiais
- Origem de campos magnéticos primordiais
- Constraints on dark energy from the observed density fluctuations spectrum
- Magnetic fields in gamma-ray burst afterglows
- The effect of a single supernova explosion on the cuspy density profile of a small-mass dark matter halo
- What is the susy mass scale?
- Precursor heating and acceleration by langmuir waves: the type ii supernova case
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas