High-Velocity Jets in Core-Collapse SNRs

Details High-Velocity Jets in Core-Collapse SNRs High-Velocity Jets in Core-Collapse SNRs

Feb 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sgrb.confe..22f&link_type=abstract

Presented at the KITP Conference: Supernova and Gamma-Ray Burst Remnants, Feb 6, 2006, Kavli Institute for Theoretical Physics,

Physics

Scientific paper

I will discuss observational evidence suggesting the presence ofhigh-velocity ejecta in the for of opposing jets in likely remnants ofcore-collapse SNe. I will concentrate on the bright radio and X-ray sourceCassiopeia A (Cas A), the youngest known supernova remnant in the MilkyWay, which shows optical jets of S-rich ejecta moving at10,000 - 15,000 km/s. While these jets are best seen in optical HSTimages, they are coincident with extended emission observed in both theX-rays and infrared.

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