  We conducted near-infrared (JHKs) imaging polarimetry toward the infrared
dark cloud (IRDC) M17 SWex, including almost all of the IRDC filaments as well
as its outskirts, with the polarimeter SIRPOL on the IRSF 1.4 m telescope. We
revealed the magnetic fields of M17 SWex with our polarization-detected sources
that were selected by some criteria based on their near-IR colors and the
column densities toward them, which were derived from the Herschel data. The
selected sources indicate not only that the ordered magnetic field is
perpendicular to the cloud elongation as a whole, but also that at both ends of
the elongated cloud the magnetic field appears to bent toward its central part,
i.e., large-scale hourglass-shaped magnetic field perpendicular to the cloud
elongation. In addition to this general trend, the elongations of the
filamentary subregions within the dense parts of the cloud appear to be mostly
perpendicular to their local magnetic fields, while the magnetic fields of the
outskirts appear to follow the thin filaments that protrude from the dense
parts. The magnetic strengths were estimated to be ~70-300 microG in the
subregions, of which lengths and average number densities are ~3-9 pc and
~2-7x10^3 cm^{-3}, respectively, by the Davis-Chandrasekhar-Fermi method with
the angular dispersion of our polarization data and the velocity dispersion
derived from the C^{18}O (J=1-0) data obtained by the Nobeyama 45 m telescope.
These field configurations and our magnetic stability analysis of the
subregions imply that the magnetic field have controlled the
formation/evolution of the M17 SWex cloud.
