On the source of dense outflows from T Tauri stars -I. Photoionization of cool MHD disc winds

Monthly Notices of the Royal Astronomical Society

Volumn 342, Issue 2, 2003, Pages 427-438

  Ferro Fontan C ^a,b   Gómez de Castro, Ana I ^b  

^a UNIVERSIDAD DE BUENOS AIRES   (Argentina)

^b UNIVERSIDAD COMPLUTENSE DE MADRID   (Spain)

Author keywords

MHD; Stars: Pre main sequence; Stars: Winds, outflows

Indexed keywords

MAGNETOPLASMA; PHOTOIONIZATION; STARS; WIND;

ACCRETION RATE; KEYS PARAMETERS; MAGNETIC FORCE; MATHEMATICAL ASPECTS; SELF-SIMILAR; STARS: PRE-MAIN SEQUENCE; STARS: WINDS OUTFLOWS; T TAURI STARS; TIDAL FORCES; Μ-MEASURE;

MAGNETOHYDRODYNAMICS;

EID: 0142073701     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06518.x     Document Type: Article

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