Chandra observation of the hard X-ray feature in IC 443

Details Chandra observation of the hard X-ray feature in IC 443 Chandra observation of the hard X-ray feature in IC 443

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..565..337c&link_type=abstract

YOUNG SUPERNOVA REMNANTS: Eleventh Astrophysics Conference. AIP Conference Proceedings, Volume 565, pp. 337-340 (2001).

Astronomy and Astrophysics

Astrophysics

Supernova Remnants, X-Ray Sources, X-Ray Bursts, Magnetohydrodynamics And Plasmas

Scientific paper

We present new Chandra A01 data of the hard X-ray feature along the southern edge of the SNR IC443. With only 10 ks of observation time we were able to extract high resolution (~1'') images that reveal a soft point source embedded in a hard comet-shaped nebula. The background-subtracted spectrum of the point source is best fit with an absorbed black body model of temperature and surface area kT=0.1+/-0.1 keV and A=0.02-0.02+0.01(d/1.5 kpc)2 km2, respectively. .

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