Modeling the magnetic field in the protostellar source NGC 1333 IRAS 4A

Astronomy and Astrophysics

Volumn 490, Issue 3, 2008, Pages

  Goncalves J ^a   Galli, D ^b   Girart, J M ^c  

^a UNIVERSITY OF LISBON   (Portugal)

^b INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^c UNIVERSITAT AUTÒNOMA DE BARCELONA   (Spain)

Author keywords

ISM: magnetic fields; Magnetohydrodynamics (MHD); Polarization; Stars: formation

Indexed keywords

CLOUDS; POLARIZATION; STARS;

HIGH ANGULAR RESOLUTIONS; ISM: MAGNETIC FIELDS; LOW-MASS PROTOSTAR; MAGNETIC FIELD DISTRIBUTION; POLARIZED EMISSIONS; SOLAR TYPE STARS; STARS: FORMATION; STOKES PARAMETERS;

MAGNETOHYDRODYNAMICS;

EID: 54949121450     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810861     Document Type: Article

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