Impact of Tangled Magnetic Fields on Star Formation

[1]  R. Klessen,et al.  Importance of the initial conditions for star formation - III. Statistical properties of embedded protostellar clusters , 2011, 1111.5440.

[2]  B. Wandelt,et al.  MAGNETIC FIELDS IN INTERSTELLAR CLOUDS FROM ZEEMAN OBSERVATIONS: INFERENCE OF TOTAL FIELD STRENGTHS BY BAYESIAN ANALYSIS , 2010 .

[3]  R. Klessen,et al.  Importance of the Initial Conditions for Star Formation - I. Cloud Evolution and Morphology , 2010, 1008.5255.

[4]  R. Klessen,et al.  MODELING COLLAPSE AND ACCRETION IN TURBULENT GAS CLOUDS: IMPLEMENTATION AND COMPARISON OF SINK PARTICLES IN AMR AND SPH , 2010, 1001.4456.

[5]  R. Beck Galactic and extragalactic magnetic fields - a concise review , 2009 .

[6]  Qizhou Zhang,et al.  Magnetic Fields in the Formation of Massive Stars , 2009, Science.

[7]  D. Ward-Thompson,et al.  SCUBA polarization observations of the magnetic fields in the pre-stellar cores L1498 and L1517B , 2006, astro-ph/0603785.

[8]  C. Heiles,et al.  The Millennium Arecibo 21 Centimeter Absorption-Line Survey. IV. Statistics of Magnetic Field, Column Density, and Turbulence , 2005, astro-ph/0501482.

[9]  R. Klein,et al.  Embedding Lagrangian Sink Particles in Eulerian Grids , 2003, astro-ph/0312612.

[10]  D. Ward-Thompson,et al.  SCUBA Polarization Measurements of the Magnetic Field Strengths in the L183, L1544, and L43 Prestellar Cores , 2003, astro-ph/0305604.

[11]  W. Holland,et al.  First Observations of the Magnetic Field Geometry in Prestellar Cores , 2000, astro-ph/0006069.

[12]  Richard I. Klein,et al.  The Jeans Condition: A New Constraint on Spatial Resolution in Simulations of Isothermal Self-Gravitational Hydrodynamics , 1997 .

[13]  I. Bonnell,et al.  Modelling accretion in protobinary systems , 1995, astro-ph/9510149.

[14]  Alyssa A. Goodman,et al.  Optical polarization maps of star-forming regions in Perseus, Taurus, and Ophiuchus , 1990 .