Comparing star formation models with interferometric observations of the protostar NGC 1333 IRAS 4A I. Magnetohydrodynamic collapse models

Saved in:
Bibliographic Details
Published inAstronomy and astrophysics (Berlin) Vol. 535; p. A44
Main Authors FRAU, P, GALLI, D, GIRART, J. M
Format Journal Article
LanguageEnglish
Published Les Ulis EDP Sciences 01.11.2011
Subjects
Astronomy
Earth, ocean, space
Exact sciences and technology
Gravitational force
Polarization
Magnetohydrodynamics
Magnetic forces
Radio observation
Interferometric observation
Protostars
stars: formation
Submillimeter wave radiation
Theoretical model
Star formation
Intensity distribution
Dynamics
Mass ratio
magnetohydrodynamics (MHD)
Age
ISM: magnetic fields
Collapse
Critical value
Molecular clouds
Stellar formation region
Star models
Physical properties
Mass transfer
Stokes parameters
ISM: individual objects: NGC 1333 IRAS 4A
MHD model
Low-mass stars
Morphology
Circumstellar disks
Magnetic fields
Online AccessGet full text

Cover

More Information
ISSN:0004-6361
1432-0746
DOI:10.1051/0004-6361/201117813