Future research by the team will establish firm links between the physics of the atmospheres and environments of the most massive stars in the Galaxy.
Now, I'm wondering if some enterprising galactic astrophysicist has said to himself, "Hmm...if this is true for hot stars, might the same physics hold for galactic spiral arms?"
Of course, it isn't established that there is any similarity between hot star spirals and galactic spirals, but wouldn't it be fascinating to investigate the possibility?
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