Origin of Molecular Outflow Determined from Thermal Dust Polarization TOMISAKA, Kohji (NAOJ) As the origin of molecular outflows ejected from protostars, there are two major explanations: magnetic - Protostars - Document - PDFSEARCH.IO

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	Origin of Molecular Outflow Determined from Thermal Dust Polarization TOMISAKA, Kohji (NAOJ) As the origin of molecular outflows ejected from protostars, there are two major explanations: magnetic Add to Reading List Document Date: 2012-07-25 04:23:18 Open Document File Size: 430,97 KB Share Result on Facebook IndustryTerm outer molecular gas / / Organization African Union / / Technology radiation / simulation / / SocialTag Broadcast engineering Electromagnetic radiation Polarization Magnetic field Toroidal and poloidal Madison Symmetric Torus Circular polarization Physics Electromagnetism Magnetism

Origin of Molecular Outflow Determined from Thermal Dust Polarization TOMISAKA, Kohji (NAOJ) As the origin of molecular outflows ejected from protostars, there are two major explanations: magneticAdd to Reading List