Radio hot SPOT in supernova remnant G 109.1-1.0

Details Radio hot SPOT in supernova remnant G 109.1-1.0 Radio hot SPOT in supernova remnant G 109.1-1.0

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986cajph..64..479g&link_type=abstract

(Conference on Jets from Stars and Galaxies, Toronto, Canada, June 24-27, 1985) Canadian Journal of Physics (ISSN 0008-4204), vo

Astronomy and Astrophysics

Astronomy

1

Pulsars, Radio Sources (Astronomy), Supernova Remnants, Astronomical Maps, Radiant Flux Density, X Ray Binaries

Scientific paper

High-resolution, Very Large Array observations of a radio hot spot in the supernova remnant G 109.1-1.0 were carried out in January 1981 and August 1984 at 6 and 20 cm to examine the possible relationship of this source to the remnant and nearby binary X-ray pulsar. The structure, spectrum, and absence of variability over a 3-year time span are consistent with a background quasar or galaxy. The source, 2258+586, exhibits an unresolved core that is self-absorbed at 20 cm and a one-sided jet. A very faint object appears on the red print of the Palomar sky survey, 3.7±1.7 arcsec from the unresolved core.

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