The super-alfvénic model of molecular clouds: Predictions for mass-to-flux and turbulent-to-magnetic energy ratios

Astrophysical Journal

Volumn 702, Issue 1 PART 2, 2009, Pages

  Lunttila, Tuomas ^a   Padoan, Paolo ^b   Juvela, Mika ^a   Nordlund, Åke ^c  

^a UNIVERSITY OF HELSINKI   (Finland)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c Astronomical Observatory/Niels Bohr Institute ^*  (Denmark)

Author keywords

ISM: magnetic fields; MHD; Radiative transfer; Stars: formation

Indexed keywords

EID: 77949498958     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/702/1/L37     Document Type: Article

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