Information for "Astronomy:Horizontal branch"

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Display titleAstronomy:Horizontal branch
Default sort keyHorizontal Branch
Page length (in bytes)15,464
Namespace ID3024
NamespaceAstronomy
Page ID568173
Page content languageen - English
Page content modelwikitext
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Page imageM5 colour magnitude diagram.png
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Page creatorimported>WikiEd2
Date of page creation10:29, 6 February 2024
Latest editorimported>WikiEd2
Date of latest edit10:29, 6 February 2024
Total number of edits1
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The horizontal branch (HB) is a stage of stellar evolution that immediately follows the red-giant branch in stars whose masses are similar to the Sun's. Horizontal-branch stars are powered by helium fusion in the core (via the triple-alpha process) and by hydrogen fusion (via the CNO cycle) in a shell...
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