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Seems that not much gets posted here lately. The link is to a simple chart that answers (in advance) some of the questions asked here. Note in particular the abundance label at the bottom of each class, with M Class stars being 80% !
See how few of the biggies (Class O, B and A) are either (1) left from original formation or (2) forming in current H2 clouds of starbirth. That same,short lifespan carries down to the very small abundance of the Supergiants.
http://anzwers.org/free/universe/startype.html
See how few of the biggies (Class O, B and A) are either (1) left from original formation or (2) forming in current H2 clouds of starbirth. That same,short lifespan carries down to the very small abundance of the Supergiants.
http://anzwers.org/free/universe/startype.html