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How Do Molecules Form in Space?

13 October 2015


The destruction of the first Population III stars in spectacular supernovas sprinkles interstellar space with clouds of heavy chemical elements. These clouds are drawn together by gravity, producing a second generation of smaller, longer-lived Population II stars. Many stars visible in the night sky are of this type.

This is the fifth in a series of posts on the Oxford University Press TUMBLR site.

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