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- Q1358411 subject Q6441178.
- Q1358411 subject Q7033768.
- Q1358411 subject Q7139523.
- Q1358411 subject Q7214315.
- Q1358411 subject Q8509164.
- Q1358411 abstract "The red clump is a feature in the Hertzsprung–Russell diagram of stars. The red clump is considered the metal-rich counterpart to the horizontal branch. Stars in this part of the Hertzsprung–Russell diagram are sometimes called clump giants. These stars are more luminous than main sequence stars of the same surface temperature (or colder than main sequence stars of comparable luminosity), or above and to the right of the main sequence on the Hertzsprung–Russell diagram. This period in a star's evolution corresponds to the core helium-burning phase, whereas the main sequence is the core hydrogen-burning phase.In theory, the absolute luminosities of stars in the red clump are fairly independent of stellar composition or age so that consequently they make good standard candles for estimating astronomical distances both within our galaxy and to nearby galaxies and clusters.An example of a red clump giant is the star Epsilon Tauri.".
- Q1358411 thumbnail Stellar_evolutionary_tracks-en.svg?width=300.
- Q1358411 wikiPageExternalLink RedClump.
- Q1358411 wikiPageWikiLink Q105902.
- Q1358411 wikiPageWikiLink Q217030.
- Q1358411 wikiPageWikiLink Q3270143.
- Q1358411 wikiPageWikiLink Q3450.
- Q1358411 wikiPageWikiLink Q405857.
- Q1358411 wikiPageWikiLink Q50076.
- Q1358411 wikiPageWikiLink Q50089.
- Q1358411 wikiPageWikiLink Q523.
- Q1358411 wikiPageWikiLink Q618164.
- Q1358411 wikiPageWikiLink Q6441178.
- Q1358411 wikiPageWikiLink Q6472.
- Q1358411 wikiPageWikiLink Q7033768.
- Q1358411 wikiPageWikiLink Q7139523.
- Q1358411 wikiPageWikiLink Q7214315.
- Q1358411 wikiPageWikiLink Q8509164.
- Q1358411 comment "The red clump is a feature in the Hertzsprung–Russell diagram of stars. The red clump is considered the metal-rich counterpart to the horizontal branch. Stars in this part of the Hertzsprung–Russell diagram are sometimes called clump giants. These stars are more luminous than main sequence stars of the same surface temperature (or colder than main sequence stars of comparable luminosity), or above and to the right of the main sequence on the Hertzsprung–Russell diagram.".
- Q1358411 label "Red clump".
- Q1358411 depiction Stellar_evolutionary_tracks-en.svg.