The Peculiar X-Ray Morphology of the Supernova Remnant G292.0+1.8 - Evidence for an Asymmetric Supernova Explosion

A high resolution X-ray image from the Einstein Observatory of the young supernova remnant G292.0+1.8 (MSH11-54) shows an unusual X-ray morphology. The remnant consists of a central bar-like feature superposed on an ellipsoidal disc of approximately uniform surface brightness. The authors attribute the bar emission to a ring of oxygen-rich material ejected in the equatorial plane of a massive rotating progenitor, and the uniform disc component to emission from material with roughly cosmic composition heated by the accompanying blast wave. This interpretation provides observational support for the rotating precursor model of a Type II supernova dicussed by Bodenheimer and Woosley.