Deep H Photography of the Vela and Puppis Supernovae Remnants

Abstract
A deep Hα photograph with the SRC 48-in. Schmidt telescope of the Vela X and Y and Puppis A radio sources has revealed many new nebulosities. It is presented here with enlargements of particular features. Correlations between these nebulosities, non-thermal radio sources, X-ray sources and the Vela pulsar are discussed.

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