Around the Pair Instability Valley - Massive SN Progenitors

Details Around the Pair Instability Valley - Massive SN Progenitors Around the Pair Instability Valley - Massive SN Progenitors

2008-05-26

arxiv.org/abs/0805.3874v1

Astronomy and Astrophysics

Astrophysics

4 pages, 3 figures, to appear in proceedings of IAU symp. no. 252 - The art of modeling stars in the 21st century, Sanya, Chin

Scientific paper

10.1017/S1743921308023120

The discovery of the extremely luminous supernova SN 2006gy, possibly
interpreted as a pair instability supernova, renewed the interest in very
massive stars. We explore the evolution of these objects, which end their life
as pair instability supernovae or as core collapse supernovae with relatively
massive iron cores, up to about $3 M_\odot$.

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