Upstream heating of shock in accretion columns of am herculis type binaries by alfven waves (1991)
- Authors:
- USP affiliated authors: OPHER, REUVEN - IAG ; PEREIRA, VERA JATENCO SILVA - IAG
- Unidade: IAG
- Assunto: ASTRONOMIA
- Language: Inglês
- Imprenta:
- Publisher: Cnpq/Fapesp/Finesp
- Publisher place: Santos
- Date published: 1991
- Source:
- Título: Resumos
- Conference titles: Congresso Brasileiro de Física dos Plasmas
-
ABNT
JATENCO-PEREIRA, Vera e OPHER, Reuven. Upstream heating of shock in accretion columns of am herculis type binaries by alfven waves. 1991, Anais.. Santos: Cnpq/Fapesp/Finesp, 1991. . Acesso em: 03 mar. 2026. -
APA
Jatenco-Pereira, V., & Opher, R. (1991). Upstream heating of shock in accretion columns of am herculis type binaries by alfven waves. In Resumos. Santos: Cnpq/Fapesp/Finesp. -
NLM
Jatenco-Pereira V, Opher R. Upstream heating of shock in accretion columns of am herculis type binaries by alfven waves. Resumos. 1991 ;[citado 2026 mar. 03 ] -
Vancouver
Jatenco-Pereira V, Opher R. Upstream heating of shock in accretion columns of am herculis type binaries by alfven waves. Resumos. 1991 ;[citado 2026 mar. 03 ] - Aceleração de partículas a energias > '10 POT.15' e v em explosões de supernovas i e ii em tempos '< OU =' 100 s
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- Mass loss in late-type stars due to radiation pressure, grains and alfven waves
- Formation of quasar clouds by thermal instability in the presence of alfven wave heating
- Some results of thermal instability in astrophysical plasmas
- Aquecimento da região pré-choque em colunas de acresção de estrelas anas-brancas magnetizadas através das ondas alfven
- The possibility of thermal instability in early-type stars due to Alfven waves
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