Effect of molecules, grains and alfven waves in the stellar winds of late-type stars (1994)
- Autores:
- Autores USP: OPHER, REUVEN - IAG ; PEREIRA, VERA JATENCO SILVA - IAG
- Unidade: IAG
- Assuntos: ASTRONOMIA; ASTROFÍSICA ESTELAR
- Idioma: Inglês
- Imprenta:
- Editora: Niels Bohr Institute
- Local: Copenhagen
- Data de publicação: 1994
- Fonte:
- Título do periódico: Proceedings
- Nome do evento: 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: 23 abr. 2024. -
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 2024 abr. 23 ] -
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 2024 abr. 23 ] - Heating of preshock region in accretion columns of am herculis
- Formation of quasar emission-line clouds by thermal instability in the presence of alfven wave heating
- Formation of extragalactic jets by alfven waves
- Protostellar Jets: numerical simulations
- Thermal instability and Alfvén waves in the formation of quasar clouds
- MHD waves in stellar winds and accretion disks
- Thermal instability in the wind of wolf-rayet stars
- Upstream heating of shock in accretion columns of am herculis type binaries by alfven waves
- Influência da abundância química sobre um vento solar impulsionado por ondas alfven
- Bipolar outflow and turbulence in molecular clouds due to protostellar alfven waves
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