Abstract:We report on the near-infrared polarimetric observations of G11.11-0.12 with the 1.4 m IRSF telescope. The starlight polarization of the background stars reveals the magnetic fields in the envelope of G11.11-0.12, which are consistent in orientation with the magnetic fields obtained from submillimeter dust polarization. The magnetic fields in G11.11-0.12 are perpendicular to the filament in a large column density range, independent of the relative orientations of G11.11-0.12. The field strength on the plane of… Show more
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