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Showing 1 to 1 of 1 for “"type IIn"”.
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Analyzing Spectra of Type Iin Supernovae and their Host Environments To Determine If Some Arise From Runaway Progenitors
We have analyzed observations of Type IIn supernovae taken by the DEIMOS spectrograph on Keck II in order to determine if there is a signicant offset in the peak of the SN H-alpha emission with respect to the predicted H-alpha peak wavelength of the host galaxy at the SN position along the slit. An …