Linked from

The 13 pages that link to Spectral energy distribution, each with the reason it gives.

• Protoplanetary diskRelated: Infrared excess in a young star's spectrum can signal a surrounding disk.

• Hertzsprung–Russell diagramRelated: It provides a fuller description of stellar radiation than a single plotted coordinate.

• ProtostarRelated: Its infrared excess helps identify embedded protostars and estimate their properties.

• Inverse Compton scatteringRelated: Its high-energy component can reveal the strength and seed photons of inverse Compton emission.

• Color indexNarrower topic: A color index compresses information from a full spectrum into two band measurements.

• Debris diskRelated: An infrared excess in this distribution is a standard way to identify debris disks.

• Photometric systemNarrower topic: A source’s spectrum determines its measured flux in each band.

• Spectral classificationCompared with: A continuous energy curve describes broad spectral shape, while classification often uses diagnostic features.

• Bolometric luminosityRelated: Integrating this distribution across wavelengths yields bolometric luminosity.

• Luminous infrared galaxyRelated: Its infrared peak and overall shape help distinguish heating sources and estimate luminosity.

• Herbig Ae/Be starRelated: Interpreting its infrared excess helps separate disk properties from stellar emission and extinction.

• Circumstellar discRelated: Its infrared excess can reveal warm dust surrounding a star.

• Young stellar objectRelated: Its infrared excess helps identify circumstellar dust and estimate evolutionary stage.