Simulations of winds of weak-lined T Tauri stars: the magnetic field geometry and the influence of the wind on giant planet migration (2009)
- Authors:
- Autor USP: PEREIRA, VERA JATENCO SILVA - IAG
- Unidade: IAG
- Subjects: CAMPO MAGNÉTICO; MÉTODOS NUMÉRICOS; MAGNETOHIDRODINÂMICA; PLANETAS; SATÉLITES; ESTRELAS T TAURI; ESTRELAS; VENTO
- Language: Inglês
- Imprenta:
- Source:
- Título: The Astrophysical Journal
- ISSN: 0004-637X
- Volume/Número/Paginação/Ano: v.703, p. 1734-1742, 2009
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ABNT
VIDOTTO, A.A et al. Simulations of winds of weak-lined T Tauri stars: the magnetic field geometry and the influence of the wind on giant planet migration. The Astrophysical Journal, v. 703, p. 1734-1742, 2009Tradução . . Acesso em: 19 fev. 2026. -
APA
Vidotto, A. A., Opher, M., Pereira, V. J., & Gombosi, T. I. (2009). Simulations of winds of weak-lined T Tauri stars: the magnetic field geometry and the influence of the wind on giant planet migration. The Astrophysical Journal, 703, 1734-1742. -
NLM
Vidotto AA, Opher M, Pereira VJ, Gombosi TI. Simulations of winds of weak-lined T Tauri stars: the magnetic field geometry and the influence of the wind on giant planet migration. The Astrophysical Journal. 2009 ;703 1734-1742.[citado 2026 fev. 19 ] -
Vancouver
Vidotto AA, Opher M, Pereira VJ, Gombosi TI. Simulations of winds of weak-lined T Tauri stars: the magnetic field geometry and the influence of the wind on giant planet migration. The Astrophysical Journal. 2009 ;703 1734-1742.[citado 2026 fev. 19 ] - Damping of alfvén waves as a heating source in protostellar accretion discs
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