Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....87..255m&link_type=abstract
Astronomy and Astrophysics, vol. 87, no. 3, July 1980, p. 255-260. Research supported by the Alexander von Humboldt-Stiftund an
Astronomy and Astrophysics
Astronomy
14
Radio Astronomy, Radio Sources (Astronomy), Stellar Radiation, Supernova Remnants, Astronomical Maps, Asymmetry, Background Radiation, High Resolution, Point Sources, Polarization Characteristics, Polarized Radiation, Radiant Flux Density, Radio Telescopes
Scientific paper
The supernova remnant G 84.2-0.8 has been mapped with the Westerbork Synthesis Radio Telescope at 1,415 MHz with a resolution of approximately 25 arcsec, and with the 100-m Effelsberg telescope at 2,695 MHz with a resolution of 4.4 arcmin. Striking filamentary structure is observed at 1,415 MHz, which appears to be aligned parallel to the major axis of the remnant and to the galactic plane. A strong asymmetry in the observed polarized flux density distribution may be related to this filamentary structure. The possibility of a physical association between the SNR and a relatively strong point source located within its boundary is discussed.
Matthews Henry E.
Shaver Peter A.
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