| http://www.w3.org/ns/prov#value | - It???s a relationship b/w the gas and the temperature of the star.What you should be anticipating now is that for stars with a range of temperatures we???re going to see black body shapes changing, peaking from red to blue, and the absorption spectra will change.Spectral classification of stars???different types of stars show different, characteristic sets of absorption lines.
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