Preliminaries Part II. Stars The radiation from stars is approximately thermal (black-body). F = T 4 = 4 R2 L The effective temperature, Teff, of a star is the temperature of a blackbody of some radius that emits the mea - Black-body radiation - Document - PDFSEARCH.IO

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	Preliminaries Part II. Stars The radiation from stars is approximately thermal (black-body). F = T 4 = 4 R2 L The effective temperature, Teff, of a star is the temperature of a blackbody of some radius that emits the mea Add to Reading List Document Date: 2012-08-07 21:07:30 Open Document File Size: 3,76 MB Share Result on Facebook

Preliminaries Part II. Stars The radiation from stars is approximately thermal (black-body). F = T 4 = 4 R2 L The effective temperature, Teff, of a star is the temperature of a blackbody of some radius that emits the meaAdd to Reading List