As the shock ploughs into material lost from the progenitor star after the initial supernova explosion, instabilities left in its wake cause the swept-up gas to fragment into clumps. The Hubble data also show thin filaments of gas. These filaments reveal where the shock wave is encountering lower...
By ASHESH DAS RUP
Location: Kepler's SN, Ophiuchus Constellation
Tags: Hubble, Space, Ophiuchus, Universe, Nebulae, ESA