The non-isothermal stage of magnetic star formation - II. Results

Physics & Astronomy

• magnetic stars 100%
• ambipolar diffusion 76%
• star formation 63%
• ohmic dissipation 51%
• hydrostatics 37%
• decoupling 35%
• magnetic flux 31%
• contraction 21%
• fragments 19%
• radii 14%
• molecular clouds 12%
• electric charge 12%
• radiative transfer 11%
• electric current 11%
• magnetic fields 11%
• fragmentation 10%
• field strength 10%
• chemistry 9%
• luminosity 8%
• geometry 6%
• electrons 4%
• simulation 4%
• temperature 3%

Earth & Environmental Sciences

• hydrostatics 44%
• dissipation 37%
• luminosity 16%
• fragmentation 12%
• geometry 9%
• simulation 6%
• temperature 5%
• effect 3%