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44Ti Emission from Cassiopeia A - SRON

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Nuclear decay and expected yields of 44 Ti<br />

High 44 Ti yields: - Low mass stars,<br />

- More energetic explosion,<br />

- Asymmetric explosion,<br />

- Low mass cut<br />

44 Ti <strong>Emission</strong> <strong>from</strong> <strong>Cassiopeia</strong> A<br />

Jacco Vink Estec, Noordwijk, January 19, 2005

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