Explain how giant molecular clouds give rise to spiral tracers as they move through a disk with spiral density waves

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A spiral density wave is a stable concentration of interstellar gas and dust. Clouds of gas and dust moving at different orbital velocities approach the dense area of the wave and collide with the material in the density wave. This collision increases mass density and triggers star formation.
The young stars created in this process will include O and B stars, which will make the arms visible with their high luminosity. The OB associations will create emission nebulae, causing a wave of star formation. The newly-formed stars will continue on the orbital track of the original cloud, passing through the leading edge of the density wave and continuing through the disk. The short-lived O and B stars will go through their entire evolutionary cycle before exiting the area of the density wave, so they are only seen in the region of the wave.

Physics & Space Science

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Physics & Space Science

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Physics & Space Science

White dwarfs are relatively

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Physics & Space Science