Solving the mystery of Type IIn supernovae

Details Solving the mystery of Type IIn supernovae Solving the mystery of Type IIn supernovae

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cxo..prop.2825c&link_type=abstract

Chandra proposal ID #11500430

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Scientific paper

X-ray observations of young supernovae provide unique constraints on the circumstellar density, profile, and elemental composition of the ejecta. Fingerprinting the exploded ejecta composition through X-ray spectroscopy can give clues to the mass and progenitor mass loss history of the exploding star. Both of these will help in understanding the relation of Type IIn progenitors to those of other classes of supernovae.

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