Other
Scientific paper
Mar 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ssrv...66..425w&link_type=abstract
Space Science Reviews, Volume 66, Issue 1-4, pp. 425-437
Other
3
Stars, Supernovae
Scientific paper
We review the possible evolutionary paths from massive stars to explosive endpoints as various types of supernovae associated with Population I and hence with massive stars: Type II-P, Type II-L, Type Ib, Type Ic, and the hybrid events SN 1987K and SN 1993J. We identify SN 1954A as another hybrid event from the evidence for both H and He in its spectrum with velocities nearly the same as SN 1983J. Evidence for ejected56Ni mass of ˜0.07 M&sun; suggests that SN II-P underwent standard iron core collapse, not collapse of an O-Ne-Mg core nor thermonuclear explosion of a C-O core. Most SN II-P presumably arise in single stars or wide binaries of ˜10 20 M&sun;. There may be indirect evidence for duplicity in some cases in the form of strong Ba II lines, such as characterized SN 1987A. SN II-L are recognizably distinct from typical SN II-P and must undergo a significantly different evolution. Despite indications that SN II-L have small envelopes that may be helium enriched, they are also distinct from events like SN 1993J that must have yet again a different evolution. The SN II-L that share a common Luminosity seem to have ejected a small nickel mass and hence may come from stars with O-Ne-Mg cores. The amount of nickel ejected by the exceptionally bright events, SN 1980K and SN 1979C, remains controversial. SN Ib require the complete loss of the H envelope, either to a binary companion or to a wind. The few identified have relatively large ejecta masses. It is not clear what evolutionary processes distinguish SN Ib's evolving in binary systems from hybrid events that retain some H in the envelope. SN Ic events are both H and He deficient. Binary models that can account for transfer of an extended helium envelope from low mass helium cores, ˜2 to 4 M&sun;, imply C-O core masses that are roughly consistent with that deduced from the ejecta mass plus a neutron star, ˜2 to 3 M&sun;. It is possible that the hybrid events are the result of Roche lobe overflow and that the “pure” events, SN Ib or SN Ic, result from common envelope evolution.
Swartz Douglas A.
Wheeler Justin C.
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