A&A 469, 1003-1004 (2007)
DOI: 10.1051/0004-6361:20066001e
Erratum
X. H. Sun1 - J. L. Han1 - W. Reich2 - P. Reich2 - W. B. Shi1 - R. Wielebinski2 - E. Fürst2
1 - National Astronomical Observatories, Chinese Academy of
Sciences, Jia-20 Datun Road, Chaoyang District, Beijing 100012,
PR China
2 - Max-Planck-Institut für Radioastronomie,
Auf dem Hügel 69, 53121 Bonn, Germany
A&A 463, 993-1007 (2007), DOI: 10.1051/0004-6361:20066001
Key words: surveys - polarization - radio continuum: general - methods: observational - ISM: supernovae remnants - errata, addenda
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Figure 3:
Gray-scale images of the polarized intensity (PI) with overlaid
bars for every third pixel in the B-field direction (polarization angle
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Open with DEXTER |
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Figure 9:
HII region G124.9+0.1: polarized intensity is
gray-scale coded, H![]() ![]() |
Open with DEXTER |
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Figure 13:
The same as Fig. 9 but for the region
encompassing the extended ojbects Sh 183, G124.0+1.4 and G122.7+1.5.
The H![]() |
Open with DEXTER |