,The structure of a type-II supernova remnant G 160.5 + 2.8 /HB-9/ observed at lambda = 12m

Details ,The structure of a type-II supernova remnant G 160.5 + 2.8 /HB-9/ observed at lambda = 12m ,The structure of a type-II supernova remnant G 160.5 + 2.8 /HB-9/ observed at lambda = 12m

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..88..299a&link_type=abstract

Astrophysics and Space Science, vol. 88, no. 2, Dec. 1982, p. 299-306.

Astronomy and Astrophysics

Astronomy

1

Brightness Distribution, Radio Sources (Astronomy), Supernova Remnants, Fine Structure, Pulsars, Radio Emission, Radio Telescopes

Scientific paper

Two-dimensional brightness distribution measurements of the old SNR G 160.5 + 2.8, at 25 MHz, show a distinctly pronounced and almost spherical envelope while individual features located near the internal boundary of the source are observable. The validation of the suggestion that the brightest feature in the decameter range might be of extragalactic origin is considered. The velocity of the pulsar PSR 0459 + 47 projected on G 160.5 + 2.8, is estimated on the basis of structure considerations, and found to not contradict the hypothesis of Damashek et al (1978) concerning the possibility of a genetic relation between the present SNR and PSR 0459 + 47.

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