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- Infrared_excess 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.".
- Infrared_excess wikiPageID "11633005".
- Infrared_excess wikiPageRevisionID "582921740".
- Infrared_excess hasPhotoCollection Infrared_excess.
- Infrared_excess subject Category:Observational_astronomy.
- Infrared_excess 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. 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.".
- Infrared_excess label "Excès d'infrarouge".
- Infrared_excess label "Infrared excess".
- Infrared_excess label "Infrarotexzess".
- Infrared_excess label "紅外過量".
- Infrared_excess label "赤外超過".
- Infrared_excess sameAs Infrarotexzess.
- Infrared_excess sameAs Excès_d'infrarouge.
- Infrared_excess sameAs 赤外超過.
- Infrared_excess sameAs m.02rm6cd.
- Infrared_excess sameAs Q1396651.
- Infrared_excess sameAs Q1396651.
- Infrared_excess wasDerivedFrom Infrared_excess?oldid=582921740.
- Infrared_excess isPrimaryTopicOf Infrared_excess.