NEBULAE · 2011-09-28

The Pacman Nebula

The Pacman Nebula combines high-energy X-rays with infrared observations of the same region.

The Pacman Nebula
X-ray: NASA/CXC/CfA/S.Wolk; IR: NASA/JPL/CfA/S.Wolk / JPL

What to observe

  • Isolate the purple structures from the red, green and blue field.
  • Look for places where X-ray and infrared features coincide.

Explanation

The source combines Chandra X-ray data with Spitzer infrared observations of the star cluster and nebula.

Color method

X-rays are mapped to purple; Spitzer infrared observations are mapped across red, green and blue.

Why it matters

A composite can compare different energy regimes without forcing them into separate images.

Sources and credits

Asset credit: X-ray: NASA/CXC/CfA/S.Wolk; IR: NASA/JPL/CfA/S.Wolk / JPL

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