Last Update 2018/01/26
I have been working on the close environments of supernovae, to search for the clues on the physical properties of the progenitor stars. For this purpose, I used the technique called integral field spectroscopy, which enables the observations of the supernova explosion sites in both spatial and spectral dimensions simultaneously. This provides an insight never obtained before into the immediate surroundings and the parent stellar populations of the supernova progenitor stars.
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