Magnetic field structure in W51A (Chrysostomou+, 2002)

Details Magnetic field structure in W51A (Chrysostomou+, 2002) Magnetic field structure in W51A (Chrysostomou+, 2002)

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ycat..33851014c&link_type=abstract

VizieR On-line Data Catalog: J/A+A/385/1014. Originally published in: 2002A&A...385.1014C

Physics

Interstellar Medium, Polarization, Magnetic Fields, Radio Lines

Scientific paper

We present 850μm imaging polarimetry of the W51A massive star forming region performed with SCUBA on the James Clerk Maxwell Telescope (JCMT) situated close to the summit of Mauna Kea, Hawaii, on the night 6 October 2000. Positions, fluxes and polarimetry of the data points shown in Fig. 1 of the paper are reported in the file table2.dat. The positional offsets are given relative to W51d (19:23:39.0, +14:31:08, J2000). All fluxes (including the Stokes Q and U parameters) are given in units of Jy/beam. The position angles give the direction of the E-vector. (1 data file).

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