The spectrum of the remnant of Kepler's supernova of 1604

Details The spectrum of the remnant of Kepler's supernova of 1604 The spectrum of the remnant of Kepler's supernova of 1604

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....86..155v&link_type=abstract

Astronomy and Astrophysics, vol. 86, no. 1-2, June 1980, p. 155, 156.

Astronomy and Astrophysics

Astrophysics

5

Line Spectra, Stellar Spectra, Supernova Remnants, Astronomical Models, Envelopes, Shock Wave Interaction

Scientific paper

A new deep spectrum of the remnant of Kepler's supernova of 1604
exhibits limes of H, He I, He II, Ca II, Mg I, [N I], [O II], [O III],
[Ne III], [Fe II], and [Fe III]. The observed spectrum is
qualitatively consistent with a model in which the circumstellar
envelope of the supernova of 1604 was excited by a strong shock.

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