Very Large Array data pertaining to the hard X-ray source on the southern edge of supernova remnant IC 443

Details Very Large Array data pertaining to the hard X-ray source on the southern edge of supernova remnant IC 443 Very Large Array data pertaining to the hard X-ray source on the southern edge of supernova remnant IC 443

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..565..345w&link_type=abstract

YOUNG SUPERNOVA REMNANTS: Eleventh Astrophysics Conference. AIP Conference Proceedings, Volume 565, pp. 345-348 (2001).

Astronomy and Astrophysics

Astrophysics

Supernova Remnants, Supernova Remnants, Pulsars

Scientific paper

We present multi-frequency (λ3.5 cm, λ6 cm, and λ20 cm) Very Large Array data pertaining to the hard X-ray feature along the southern edge of the supernova remnant IC 443. They have revealed a cometary nebula blending with the shell of the remnant. Polarization images show an intriguing magnetic field structure which wraps around a point at the widest part of the cometary nebula and appears strongest where the tail blends with the shell of IC 443. The nebula has a mean flux density of 200 mJy and a spectral index much flatter than IC 443 as a whole. .

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