Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...186l...3g&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 186, no. 1-2, Nov. 1987, p. L3, L4.
Astronomy and Astrophysics
Astrophysics
11
Companion Stars, Neutron Stars, Stellar Evolution, Stellar Models, Supernova 1987A, White Dwarf Stars, Relativistic Velocity, Stellar Luminosity, Stellar Mass Accretion, Stellar Mass Ejection, Stellar Spectrophotometry, Visible Spectrum
Scientific paper
A model for the companion of SN 1987 A, observed recently by optical speckle interferometry, is proposed. It is suggested that the observed relativistic velocity and the high luminosity can be naturally explained within a framework of a rotating collapse, producing two neutron stars in a binary system which decays due to emission of gravitational radiation. This leads eventually to the tidal disruption of the less massive member and the ejection of a fraction of the disrupted star of mass of less than about 0.1 solar masses at a relativistic velocity. The decompression of the ejected fraction transforms its composition from that of nuclear matter to that of superheavy elements (z of about 126), leading to a formation of a 'white dwarf' which on its way out accretes about 0.0001 solar masses from the progenitor. The ejected mass has about 0.0003 of Ni-56 producing gamma-ray photons, by radioactive decay of Ni-56 and Co-56 that are reprocessed into the observed optical photons, in the layer accreted on the way out. In the present model there is no need for an energy source separate from the companion, as is the case with models proposed so far.
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