Main sequence

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The main sequence is the part of the H-R diagram where stars spend most of their life. While on the main sequence a star undergoes hydrogen burning in its core.
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#REDIRECT [[Stellar evolution#Main Sequence]]
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[[Category:Astronomical concept]]
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[[Category:Stubs]]
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Latest revision as of 13:58, 16 September 2010

  1. REDIRECT Stellar evolution#Main Sequence
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