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44Ti Emission from Cassiopeia A - SRON

44Ti Emission from Cassiopeia A - SRON

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The goals of Integral observations of 44 Ti<br />

●<br />

Use 44 Ti as a tracer for young supernova remnants<br />

-> M. Renaud (search)<br />

-> A. von Kienlin (Vela Jr.)<br />

●<br />

Test supernova explosion theories<br />

-> This talk<br />

-> M. Renaud (how much 44 Ti do Type Ia SNe<br />

(e.g. Tycho) produce?)<br />

●<br />

<strong>Cassiopeia</strong> A: the most certain source of 44 Ti<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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