Observations of the western part of the Cygnus Loop at 408 MHz - The 5C8 survey

Details Observations of the western part of the Cygnus Loop at 408 MHz - The 5C8 survey Observations of the western part of the Cygnus Loop at 408 MHz - The 5C8 survey

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.211..433g&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 211, Nov. 15, 1984, p. 433-441. Research supported by t

Other

28

Radio Spectra, Stellar Spectrophotometry, Supernova Remnants, Astronomical Catalogs, Cygnus Constellation, Data Reduction, Emission Spectra, Interstellar Space, Radiant Flux Density, Spectral Energy Distribution, Spectral Resolution

Scientific paper

The western part of the Cygnus Loop supernova remnant has been observed with the Cambridge One-Mile telescope at 408 MHz with a resolution of 80×160 arcsec2 (RA×Dec). These observations reveal the radio emission from the remnant in great detail, including a remarkable radio filament that stretches over much of the length of the remnant. The nature of this feature, and others, are discussed in terms of the interaction of the remnant with differing regions of the interstellar medium.

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