|home - login - register - about - sitemap|
Stellar Blackbody Radiation Curves Documents
This material has 2 associated documents. Select a document title to view a document's information.
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 November 11, 2010
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
brought to you by the AAS, AAPT, and NSF-NSDL
a member of the comPADRE Digital Library
©2003-2013, All Rights Reserved
contact the Astronomy Center
|about AstronomyCenter.org - terms - privacy - faq|