The LMC supernova in order of magnitude

Details The LMC supernova in order of magnitude The LMC supernova in order of magnitude

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989qjras..30..419m&link_type=abstract

Royal Astronomical Society, Quarterly Journal (ISSN 0035-8738), vol. 30, Dec. 1989, p. 419-429.

Physics

Magellanic Clouds, Neutron Stars, Stellar Magnitude, Supernova 1987A, Neutrinos, Nuclear Fusion, Radioactivity, Stellar Cores, Stellar Evolution, Stellar Luminosity

Scientific paper

SN 1987A is described in terms of simple physics. Observations of Sk-69 202 and SN 1987A are reviewed and a simplified explanation of the physical mechanisms involved in the evolution of SN 1987A is given. Consideration is given to stellar equilibrium and collapse, shock break-out, brightening of the supernova, energy released in the core collapse, the neutron star in SN 1987A, radioactivity in the supernova, and neutrino production and interactions.

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