Het overblijfsel van de supernova G292.0 + 1.8 bevat een pulsar die met een snelheid van meer dan een miljoen mijl per uur beweegt, zoals te zien is in de Chandra-afbeelding, samen met een optische afbeelding van de Digitized Sky Survey. Pulsars zijn snel ronddraaiende neutronensterren die kunnen ontstaan wanneer massieve sterren geen brandstof meer … Read more
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