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- Diffuse nebulae are huge clouds of gas and dust which accumulate
- in the arms of spiral galaxies. A typical diffuse nebula can be
- 50 or more light years across. When some regions of a diffuse
- nebula reach a critical density, new stars form. The bright
- nebulae which we see are usually illuminated by these young
- stars, and therefore open galactic star clusters and bright
- nebulae are often found in association (see the Pleiades display
- in the Open Cluster selection). Dark nebulae have no nearby
- stars to illuminate them, and they appear as "holes" embedded in
- the backdrop of more distant stars.