a. Does a hot, thin gas emit a continuous spectrum, a bright line spectra with gaps between the lines, or a dark line sp
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a. Does a hot, thin gas emit a continuous spectrum, a bright line spectra with gaps between the lines, or a dark line sp
a. Does a hot, thin gas emit a continuous spectrum, a bright line spectra with gaps between the lines, or a dark line spectra with all frequencies except the missing (absorbed) one? b. Why do we see dark line spectra when we look at stars?
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