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- Q1202702 subject Q6864552.
- Q1202702 abstract "CH stars are particular type of carbon stars which are characterized by the presence of exceedingly strong absorption bands due to CH (methylidyne) in their spectra. They belong to the stellar population II, meaning they're metal poor and generally pretty middle-aged stars, and are under-luminous compared to the classical C–N carbon stars. Many CH stars are known to be binaries, and it's reasonable to believe this is the case for all CH stars. Like Barium stars, they are probably the result of a mass transfer from a former classical carbon star, now a white dwarf, to the current CH-classed star.".
- Q1202702 wikiPageExternalLink CH_star.html.
- Q1202702 wikiPageWikiLink Q130019.
- Q1202702 wikiPageWikiLink Q1436016.
- Q1202702 wikiPageWikiLink Q179600.
- Q1202702 wikiPageWikiLink Q3333711.
- Q1202702 wikiPageWikiLink Q5871.
- Q1202702 wikiPageWikiLink Q6864552.
- Q1202702 wikiPageWikiLink Q808220.
- Q1202702 type Place.
- Q1202702 type CelestialBody.
- Q1202702 type Location.
- Q1202702 type Place.
- Q1202702 type Star.
- Q1202702 type Thing.
- Q1202702 comment "CH stars are particular type of carbon stars which are characterized by the presence of exceedingly strong absorption bands due to CH (methylidyne) in their spectra. They belong to the stellar population II, meaning they're metal poor and generally pretty middle-aged stars, and are under-luminous compared to the classical C–N carbon stars. Many CH stars are known to be binaries, and it's reasonable to believe this is the case for all CH stars.".
- Q1202702 label "CH star".