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1999MNRAS.304..406I - Mon. Not. R. Astron. Soc., 304, 406-414 (1999/April-1)
The magnetic field structure of the DR 21 region.
ITOH Y., CHRYSOSTOMOU A., BURTON M., HOUGH J.H. and TAMURA M.
Abstract (from CDS):
The polarimetry of the H2 v=1–0 S(1) line suggests that the magnetic field is parallel to the outflow axis for the eastern outflow lobe, whereas it appears twisted perpendicular to this axis for the western lobe. This peculiar morphology for the magnetic field may imply the presence of either a two-component magnetic field along the line of sight or a complex, wound-up magnetic field.
Abstract Copyright: 1999, Royal Astronomical Society
Journal keyword(s): magnetic fields - polarization - techniques: polarimetric - stars: pre-main-sequence - ISM: individual: DR21 - infrared: stars
Nomenclature: Fig.1: [DS96] O3 added. Table 2: [ICB99] WN (Nos E1-E5, W1-W5).
Simbad objects: 18
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