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The sequence of stellar spectral types is shown in the figure below.Explain why the hottest star (O5) has so little emission in the visible portion of the spectrum (450-700 nm), spectral types F-K show the most emission in the visible band, and still cooler stars (M type) once again show very little in the visible band.
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A graphical depiction that shows the maximum quantity of one good that can be produced for every possible quantity of another good, given the available resources and technology.
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