Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-01-28
Astronomy and Astrophysics
Astrophysics
6 pages, 4 figures, to appear in IAU Symp. 250, Massive Stars as Cosmic Engines, Kauai (HI), 12/2007, ed. F. Bresolin, P. Crow
Scientific paper
10.1017/S174392130802053X
We discuss how rotation and binary interactions may be related to the diversity of type Ibc supernovae and long gamma-ray bursts. After presenting recent evolutionary models of massive single and binary stars including rotation, the Tayler-Spruit dynamo and binary interactions, we argue that the nature of SNe Ibc progenitors from binary systems may not significantly differ from that of single star progenitors in terms of rotation, and that most long GRB progenitors may be produced via the quasi-chemically homogeneous evolution at sub-solar metallicity. We also briefly discuss the possible role of magnetic fields generated in the convective core of a massive star for the transport of angular momentum, which is potentially important for future stellar evolution models of supernova and GRB progenitors.
Cantiello Matteo
Glatzmaier Gary A.
Langer Norbert
Woosley Stan E.
Yoon S.-Ch.
No associations
LandOfFree
Evolution of progenitor stars of Type Ibc supernovae and long gamma-ray bursts does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Evolution of progenitor stars of Type Ibc supernovae and long gamma-ray bursts, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evolution of progenitor stars of Type Ibc supernovae and long gamma-ray bursts will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-184999