Magnetic fields in the formation of sun-like stars

Josep M. Girart, Ramprasad Rao, Daniel P Marrone

Research output: Contribution to journalArticle

209 Citations (Scopus)

Abstract

We report high-angular-resolution measurements of polarized dust emission toward the low-mass protostellar system MGC 1333 IRAS 4A. We show that in this system the observed magnetic field morphology is in agreement with the standard theoretical models of the formation of Sun-like stars in magnetized molecular clouds at scales of a few hundred astronomical units; gravity has overcome magnetic support, and the magnetic field traces a clear hourglass shape. The magnetic field is substantially more important than turbulence in the evolution of the system, and the initial misalignment of the magnetic and spin axes may have been important in the formation of the binary system.

Original languageEnglish (US)
Pages (from-to)812-814
Number of pages3
JournalScience
Volume313
Issue number5788
DOIs
StatePublished - Aug 11 2006
Externally publishedYes

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Solar System
Magnetic Fields
Gravitation
Dust
Theoretical Models

ASJC Scopus subject areas

  • General

Cite this

Magnetic fields in the formation of sun-like stars. / Girart, Josep M.; Rao, Ramprasad; Marrone, Daniel P.

In: Science, Vol. 313, No. 5788, 11.08.2006, p. 812-814.

Research output: Contribution to journalArticle

Girart, Josep M. ; Rao, Ramprasad ; Marrone, Daniel P. / Magnetic fields in the formation of sun-like stars. In: Science. 2006 ; Vol. 313, No. 5788. pp. 812-814.
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