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J/A+A/385/1014      Magnetic field structure in W51A       (Chrysostomou+, 2002)

The magnetic field structure in W51A Chrysostomou, A., Aitken, D.K., Jenness, T., Davis, C.J., Hough, J.H., Curran, R., Tamura, M. <Astron. Astrophys. 385, 1014 (2002)> =2002A&A...385.1014C
ADC_Keywords: Interstellar medium ; Polarization ; Magnetic fields ; Radio lines Keywords: ISM: magnetic fields - ISM: individual objects: W51A - stars: formation - techniques: polarimetric - submillimetre Description: 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. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 69 224 Positions, fluxes and polarisation of data points shown in Fig. 1.
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 5 F5.1 arcsec oRA Right ascension offset (1) 7- 11 F5.1 arcsec oDE Declination offset (1) 14- 18 F5.2 Jy I Intensity (in Jy/beam) at 850um 20- 23 F4.2 Jy e_I Intensity error (in Jy/beam) 26- 30 F5.2 Jy Q Q Stokes Intensity (in Jy/beam) 32- 35 F4.2 Jy e_Q Q Stokes intensity error (in Jy/beam) 38- 42 F5.2 Jy U U Stokes Intensity (in Jy/beam) 44- 47 F4.2 Jy e_U U Stokes intensity error (in Jy/beam) 50- 52 F3.1 % Pol Polarisation percentage 55- 57 F3.1 % e_Pol Polarisation error 60- 64 F5.1 deg PA [-90/90] Position angle of the E-vector 66- 69 F4.1 deg e_PA Position angle error
Note (1): The positional offsets are given relative to W51d. Position of W51d: RA= 19 23 39.9, DE= +14 31 08, J2000
Acknowledgements: Antonio Chrysostomou
(End) Patricia Bauer [CDS] 01-Feb-2002
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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