The possibility of thermal instability in early-type stars due to Alfven waves (1998)
- Authors:
- USP affiliated authors: PEREIRA, VERA JATENCO SILVA - IAG ; OPHER, REUVEN - IAG
- Unidade: IAG
- Subjects: ASTRONOMIA; ASTROFÍSICA ESTELAR
- Language: Inglês
- Source:
- Título do periódico: Astrophysical Journal
- Volume/Número/Paginação/Ano: v. 501, n. 2, pt. 1, p. 797-804, jul. 1998
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ABNT
GONÇALVES, D. R. e JATENCO-PEREIRA, Vera e OPHER, Reuven. The possibility of thermal instability in early-type stars due to Alfven waves. Astrophysical Journal, v. 501, n. 2, p. 797-804, 1998Tradução . . Acesso em: 29 mar. 2024. -
APA
Gonçalves, D. R., Jatenco-Pereira, V., & Opher, R. (1998). The possibility of thermal instability in early-type stars due to Alfven waves. Astrophysical Journal, 501( 2), 797-804. -
NLM
Gonçalves DR, Jatenco-Pereira V, Opher R. The possibility of thermal instability in early-type stars due to Alfven waves. Astrophysical Journal. 1998 ; 501( 2): 797-804.[citado 2024 mar. 29 ] -
Vancouver
Gonçalves DR, Jatenco-Pereira V, Opher R. The possibility of thermal instability in early-type stars due to Alfven waves. Astrophysical Journal. 1998 ; 501( 2): 797-804.[citado 2024 mar. 29 ] - Heating of preshock region in accretion columns of am herculis
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- 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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