Predicted rotation signatures in MHD disc winds and comparison to DG Tau observations

Astronomy and Astrophysics

Volumn 416, Issue 3, 2004, Pages

  Pesenti, N ^a   Dougados, C ^a   Cabrit, S ^b   Ferreira, J ^a   Casse, F ^c   Garcia, P ^d   O'Brien, D ^d  

^a LABORATOIRE D ASTROPHYSIQUE   (France)

^b OBSERVATOIRE DE PARIS   (France)

^c FOM INSTITUTE FOR PLASMA PHYSICS RIJNHUIZEN   (Netherlands)

^d CENTRO DE ASTROFÍSICA   (Portugal)

Author keywords

ISM: individual objects: DG Tau; ISM: jets and outflow; Stars: formation

Indexed keywords

APPROXIMATION THEORY; COMPUTATION THEORY; ENTROPY; IMAGING TECHNIQUES; IONIZATION; MAGNETOHYDRODYNAMICS; MATHEMATICAL MODELS;

DG TAU; FORMATION - ISM; INDIVIDUAL OBJECTS; ISM; JETS AND OUTFLOW - STARS;

ASTROPHYSICS;

EID: 1642634895     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040033     Document Type: Article

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