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Stellar Blackbody Radiation Curves Documents
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Stellar Blackbody Radiation Curves model simulates the blackbody radiation curve of stars and how this leads to the observed color and luminosity of the star. If a star can be treated as a blackbody, the blackbody radiation curve of the star, the power density per area (or intensity) per wavelength (energy/time/volume) vs wavelength, is dependent on the star's temperature (spectral class).
Last Modified August 5, 2013
This file has previous versions.
Source Code Documents
The source code zip archive contains an XML representation of the Stellar Blackbody Radiation Curves Model. Unzip this archive in your EJS workspace to compile and run this model using EJS.
Published November 11, 2010
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