esahubble_opo0429i October 6th, 2004
Credit: NASA, ESA, R. Sankrit and W. Blair (Johns Hopkins University)
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-density, more uniform interstellar material.
Provider: Hubble Space Telescope | ESA
Image Source: https://www.spacetelescope.org/images/opo0429i/
Curator: ESA/Hubble, Garching bei München, Germany
Image Use Policy: Creative Commons Attribution 4.0 International License
Detailed color mapping information coming soon...
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