Some results of thermal instability in astrophysical plasmas (1995)
- Authors:
- USP affiliated authors: OPHER, REUVEN - IAG ; PEREIRA, VERA JATENCO SILVA - IAG
- Unidade: IAG
- Subjects: ASTRONOMIA; ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Publisher: Union Astronomica Internacional
- Publisher place: Montevideo
- Date published: 1995
- Source:
- Título: Programa y Resumenes
- Conference titles: Reunion Regional Latinoamericana de Astronomia
-
ABNT
GONÇALVES, D. R. e JATENCO-PEREIRA, Vera e OPHER, Reuven. Some results of thermal instability in astrophysical plasmas. 1995, Anais.. Montevideo: Union Astronomica Internacional, 1995. . Acesso em: 26 jan. 2026. -
APA
Gonçalves, D. R., Jatenco-Pereira, V., & Opher, R. (1995). Some results of thermal instability in astrophysical plasmas. In Programa y Resumenes. Montevideo: Union Astronomica Internacional. -
NLM
Gonçalves DR, Jatenco-Pereira V, Opher R. Some results of thermal instability in astrophysical plasmas. Programa y Resumenes. 1995 ;[citado 2026 jan. 26 ] -
Vancouver
Gonçalves DR, Jatenco-Pereira V, Opher R. Some results of thermal instability in astrophysical plasmas. Programa y Resumenes. 1995 ;[citado 2026 jan. 26 ] - 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
- 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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