Large Magellanic Cloud, N44 houses numerous massive bright stars, lengthy lanes of dark dust, and vast clouds of hydrogen gas that glows red. The red color of the N44 emission nebula comes from pervasive hydrogen atoms re-acquiring electrons that were knocked away by energetic light from massive stars. The central stars also appear to have somehow created the huge superbubble visible in the lower left. N44, pictured above, spans about 1,000 light years and lies about 170,000 light years distant.
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Publications with keywords: N44C - emission nebula - LMC
Publications with words: N44C - emission nebula - LMC