Tilted winds of weak-lined T Tauri stars: 3D simulations (2010)
- Authors:
- USP affiliated authors: OPHER, REUVEN - IAG ; PEREIRA, VERA JATENCO SILVA - IAG
- Unidade: IAG
- Subjects: MEIO INTERESTELAR; ESTRELAS T TAURI; MAGNETOHIDRODINÂMICA
- Language: Inglês
- Imprenta:
- Source:
- Título: Program & Abstracts
- Conference titles: Workshop Challenges of New Physics in Space
-
ABNT
VIDOTTO, A. A et al. Tilted winds of weak-lined T Tauri stars: 3D simulations. Program & Abstracts. São Paulo: IAG-USP. Disponível em: http://www.astro.iag.usp.br/~challenges/index.html. Acesso em: 11 mar. 2026. , 2010 -
APA
Vidotto, A. A., Opher, R., Jatenco-Pereira, V., & Gombosi, T. I. (2010). Tilted winds of weak-lined T Tauri stars: 3D simulations. Program & Abstracts. São Paulo: IAG-USP. Recuperado de http://www.astro.iag.usp.br/~challenges/index.html -
NLM
Vidotto AA, Opher R, Jatenco-Pereira V, Gombosi TI. Tilted winds of weak-lined T Tauri stars: 3D simulations [Internet]. Program & Abstracts. 2010 ;[citado 2026 mar. 11 ] Available from: http://www.astro.iag.usp.br/~challenges/index.html -
Vancouver
Vidotto AA, Opher R, Jatenco-Pereira V, Gombosi TI. Tilted winds of weak-lined T Tauri stars: 3D simulations [Internet]. Program & Abstracts. 2010 ;[citado 2026 mar. 11 ] Available from: http://www.astro.iag.usp.br/~challenges/index.html - 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
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas