Gum Nebula

Gum Nebula A large, almost circular emission nebula in the constellations Vela and Puppis, discovered by the Australian astronomer Colin Stanley Gum (1924–60). The Gum Nebula is 36 ° across and is estimated to be 1300 l.y. away, which gives it a true diameter of about 800 l.y. It is expanding at 20 km/s, and is thought to have been formed by a supernova explosion over 1 million years ago. It contains the Vela OB2 association, the hot stars of which may cause it to shine. The Vela Supernova Remnant and the Vela Pulsar are embedded within the Gum Nebula, but are much younger.

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