The nickel bubble in SN1987A

Details The nickel bubble in SN1987A The nickel bubble in SN1987A

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aipc..232..257a&link_type=abstract

IN: Gamma-ray line astrophysics; Proceedings of the International Symposium, Paris, France, Dec. 10-13, 1990 (A92-43619 18-90).

Astronomy and Astrophysics

Astrophysics

1

Nickel Isotopes, Nuclear Astrophysics, Radioactive Isotopes, Supernova 1987A, Cobalt Isotopes, Magnetohydrodynamic Stability, Stellar Composition, Stellar Luminosity, Stellar Models

Scientific paper

Instabilities in SN1987A are briefly discussed. The effects of decay of
Ni-56 and Co-56 on the observed velocities, thermal luminosity, and
gamma and X-ray fluxes are emphasized. The possibility is addressed that
a new neutron star is the source of the nickel bubble observed in
SN1987A.

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