The Synthesis of44Ti and56Ni in Massive Stars
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/836/i=1/a=79/pdf
Reference36 articles.
1. Improved measurement of theTi44half-life from a 14-year long study
2. TURBULENT CONVECTION IN STELLAR INTERIORS. II. THE VELOCITY FIELD
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4. Nuclear Quasi-Equilibrium during Silicon Burning
5. 44 Ti gamma-ray emission lines from SN1987A reveal an asymmetric explosion
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