Magnetic fields in the Eos cloud are parallel to the cloud structure, sub-Alfvenic, and subcritical, with plane-of-sky strengths around 6 microgauss in Eos and 12 microgauss in the denser MBM 40 region.
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Magnetic fields in the Eos Cloud: dynamically important fields in the interface between atomic and molecular gas
Magnetic fields in the Eos cloud are parallel to the cloud structure, sub-Alfvenic, and subcritical, with plane-of-sky strengths around 6 microgauss in Eos and 12 microgauss in the denser MBM 40 region.