The supernova in the Large Magellanic Cloud - Attempting a balance after three years

Details The supernova in the Large Magellanic Cloud - Attempting a balance after three years The supernova in the Large Magellanic Cloud - Attempting a balance after three years

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990s%26w....29..438h&link_type=abstract

Sterne und Weltraum (ISSN 0039-1263), vol. 29, July-Aug. 1990, p. 438-447. In German.

Astronomy and Astrophysics

Astronomy

Hertzsprung-Russell Diagram, Light Curve, Stellar Radiation, Stellar Spectra, Supernova 1987A, Astronomical Photography, Barium, Helium, Hydrogen, Oxygen, Ultraviolet Radiation

Scientific paper

Present understanding of SN 1987A is discussed. The evolution of the progenitor star up to the supernova stage is described, and the reasons for the unusual character of the light curve are considered. Based on the supernova spectra, the chemical makeup of the supernova and the reasons for its departure from spherical symmetry are addressed. The supernova explosion mechanism is examined, including the energy source.

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