Effect of chemical abundance on a wolf-rayet stellar wind driven by radiation pressure and alfven waves (1993)
- Authors:
- USP affiliated authors: OPHER, REUVEN - IAG ; PEREIRA, VERA JATENCO SILVA - IAG
- Unidade: IAG
- Subjects: ASTRONOMIA; ASTROFÍSICA ESTELAR; ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Source:
- Título: Astronomy and Astrophysics
- Volume/Número/Paginação/Ano: v. 270, n. 1-2, p. 345-354, mar. 1993
-
ABNT
SANTOS, L C e JATENCO-PEREIRA, Vera e OPHER, Reuven. Effect of chemical abundance on a wolf-rayet stellar wind driven by radiation pressure and alfven waves. Astronomy and Astrophysics, v. 270, n. 1-2, p. 345-354, 1993Tradução . . Acesso em: 26 jan. 2026. -
APA
Santos, L. C., Jatenco-Pereira, V., & Opher, R. (1993). Effect of chemical abundance on a wolf-rayet stellar wind driven by radiation pressure and alfven waves. Astronomy and Astrophysics, 270( 1-2), 345-354. -
NLM
Santos LC, Jatenco-Pereira V, Opher R. Effect of chemical abundance on a wolf-rayet stellar wind driven by radiation pressure and alfven waves. Astronomy and Astrophysics. 1993 ; 270( 1-2): 345-354.[citado 2026 jan. 26 ] -
Vancouver
Santos LC, Jatenco-Pereira V, Opher R. Effect of chemical abundance on a wolf-rayet stellar wind driven by radiation pressure and alfven waves. Astronomy and Astrophysics. 1993 ; 270( 1-2): 345-354.[citado 2026 jan. 26 ] - Astrophysical jets: numerical simulations
- 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
- O aquecimento alfvênico em discos e colunas de acresção de estrelas T Tauri clássicas
- Possibility of grains alignment by alfven waves in the vicinity of stars
- Two-phase broad-line regions in the presence of alfven wave heating: the role of nonlinear and turbulent heating
- The fundamental role of Alfven waves in the formation of stars
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