horizontal branch
The part of the Hertzsprung-Russell diagram
of a typical globular cluster; it contains
stars with masses of 0.6 to 0.8 solar masses that are hotter and fainter
than those on the giant branch. A star
appears on the horizontal branch after it has undergone its helium
flash and begun to burn helium steadily in its core and hydrogen in
a surrounding envelope. Related category
STELLAR
ASTROPHYSICS
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