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

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Date: 2012-08-07 21:07:30		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 Source URL: people.physics.tamu.edu Download Document from Source Website File Size: 3,76 MB Share Document on Facebook