Nebulosity around Pleiades stars

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SUMMARY

The nebulosity surrounding the Pleiades stars (M45) is not a remnant of their formation but rather an unrelated dust cloud in the interstellar medium. This dust reflects the light of the hot blue and luminous stars that have formed within the last 100 million years. Initially thought to be leftover material from the cluster's formation, this phenomenon is now understood to be due to the stars passing through this interstellar dust cloud. The alternative name for the nebulosity, Maia Nebula, is derived from the star Maia, one of the brightest in the cluster.

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virgil1612
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Hello,

I'm curious about the origin of the nebulosity that can be seen around the main stars in the open cluster Pleiades (M45). Is it a residual of the huge cloud from which these stars were born not so long ago (astronomically), or it just happens that these stars pass through an interstellar cloud, which then reflects their light.

Thanks,
Virgil.
 
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Well, according to Wikipedia:
"The cluster is dominated by hot blue and extremely luminous stars that have formed within the last 100 million years. Dust that forms a faint reflection nebulosity around the brightest stars was thought at first to be left over from the formation of the cluster (hence the alternative name Maia Nebula after the star Maia), but is now known to be an unrelated dust cloud in the interstellar medium, through which the stars are currently passing. "
 
phyzguy said:
Well, according to Wikipedia:
"The cluster is dominated by hot blue and extremely luminous stars that have formed within the last 100 million years. Dust that forms a faint reflection nebulosity around the brightest stars was thought at first to be left over from the formation of the cluster (hence the alternative name Maia Nebula after the star Maia), but is now known to be an unrelated dust cloud in the interstellar medium, through which the stars are currently passing. "

Thanks phyzguy, I guess I should have checked the net myself before asking.
 

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