Effect of molecules, grains and alfven waves in the stellar winds of late-type stars (1994)
- Authors:
- USP affiliated authors: OPHER, REUVEN - IAG ; PEREIRA, VERA JATENCO SILVA - IAG
- Unidade: IAG
- Subjects: ASTRONOMIA; ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Publisher: Niels Bohr Institute
- Publisher place: Copenhagen
- Date published: 1994
- Source:
- Título: Proceedings
- Conference titles: International Astronomical Union Colloquium
-
ABNT
SANTOS, L C e JATENCO-PEREIRA, Vera e OPHER, Reuven. Effect of molecules, grains and alfven waves in the stellar winds of late-type stars. 1994, Anais.. Copenhagen: Niels Bohr Institute, 1994. . Acesso em: 11 mar. 2026. -
APA
Santos, L. C., Jatenco-Pereira, V., & Opher, R. (1994). Effect of molecules, grains and alfven waves in the stellar winds of late-type stars. In Proceedings. Copenhagen: Niels Bohr Institute. -
NLM
Santos LC, Jatenco-Pereira V, Opher R. Effect of molecules, grains and alfven waves in the stellar winds of late-type stars. Proceedings. 1994 ;[citado 2026 mar. 11 ] -
Vancouver
Santos LC, Jatenco-Pereira V, Opher R. Effect of molecules, grains and alfven waves in the stellar winds of late-type stars. Proceedings. 1994 ;[citado 2026 mar. 11 ] - Aceleração de partículas a energias > '10 POT.15' e v em explosões de supernovas i e ii em tempos '< OU =' 100 s
- Alfven-driven protostellar winds
- MHD waves in stellar winds and accretion disks
- Astrophysical jets: numerical simulations
- Effect of chemical abundance on a wolf-rayet stellar wind driven by radiation pressure and alfven waves
- 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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