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Absorption Spectra of Type II Supernovae
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1972
Year
Type Ii SupernovaeCosmic AbundancePhysicsNatural SciencesFe IiStellar StructureAbsorption SpectroscopyWavelength CoincidenceIntensity MinimaHigh-energy AstrophysicsSpectroscopic PropertyAstrophysics
On the bases of wavelength coincidence and comparison of observed and synthetic spectra, intensity minima in Type II supernova spectra are attributed to blueshifted absorption lines of hydrogen and Fe II .