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- Q1396651 subject Q6306516.
- Q1396651 abstract "An infrared excess is a measurement of an astronomical source, typically a star, that in their spectral energy distribution has a greater measured infrared flux than expected by assuming the star is a blackbody radiator. Infrared excesses are often the result of circumstellar dust and are common in young stellar objects and evolved stars on the asymptotic giant branch or older.In addition, monitoring for infrared excess emission from stellar systems is one possible method that could enable a search for large-scale stellar engineering projects of a hypothetical extraterrestrial civilization; for example a Dyson sphere or Dyson swarm.".
- Q1396651 wikiPageWikiLink Q1012875.
- Q1396651 wikiPageWikiLink Q11388.
- Q1396651 wikiPageWikiLink Q2035809.
- Q1396651 wikiPageWikiLink Q469.
- Q1396651 wikiPageWikiLink Q497654.
- Q1396651 wikiPageWikiLink Q50089.
- Q1396651 wikiPageWikiLink Q523.
- Q1396651 wikiPageWikiLink Q6306516.
- Q1396651 wikiPageWikiLink Q7280375.
- Q1396651 wikiPageWikiLink Q7575187.
- Q1396651 wikiPageWikiLink Q900097.
- Q1396651 comment "An infrared excess is a measurement of an astronomical source, typically a star, that in their spectral energy distribution has a greater measured infrared flux than expected by assuming the star is a blackbody radiator.".
- Q1396651 label "Infrared excess".