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J/A+A/503/827    6cm and 11cm polarisation maps of SNR G65.2+5.7   (Xiao+, 2009)

Radio properties of the low surface brightness SNR G65.2+5.7. Xiao L., Reich W., Furst E., Han J.L. <Astron. Astrophys. 503, 827 (2009)> =2009A&A...503..827X
ADC_Keywords: Supernova remnants ; Radio sources ; Polarization Keywords: ISM: supernova remnants - ISM: magnetic fields - radio continuum: ISM - radiation mechanisms: non-thermal Abstract: SNR G65.2+5.7 is one of few supernova remnants (SNRs) that have been optically detected. It is exceptionally bright in X-rays and the optical [O III]-line. Its low surface brightness and large diameter ensure that radio observations of SNR G65.2+5.7 are technically difficult and thus have hardly been completed. Many physical properties of this SNR, such as spectrum and polarization, can only be investigated by radio observations. Description: The λ11cm and λ6cm continuum and polarization observations of SNR G65.2+5.7 were completed with the Effelsberg 100-m and the Urumqi 25-m telescopes, respectively, to investigate the integrated spectrum, the spectral index distribution, and the magnetic field properties. Archival λ21cm data of the Effelsberg 100-m telescope were also used. Objects: ----------------------------------------------------- RA (2000) DE Designation(s) ----------------------------------------------------- 19 32.9 +31 12 SNR G65.2+5.7 = SNR G065.3+05.7 ----------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file maps.dat 74 10 List of the fits images fits/* 0 10 FITS images
See also: J/A+A/482/783 : 6cm and 11cm polarisation maps of SNR S147 (Xiao+, 2008) Byte-by-byte Description of file: maps.dat
Bytes Format Units Label Explanations
1- 17 A17 --- FileName Name of the fits file, in subdirectory fits 19- 74 A56 --- Title Title of the image
Acknowledgements: Wolfgang Reich, wreich(at)
(End) Patricia Vannier [CDS] 22-May-2009
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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