44Ti Emission from Cassiopeia A - SRON

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The goals of Integral observations of 44 Ti ● Use 44 Ti as a tracer for young supernova remnants -> M. Renaud (search) -> A. von Kienlin (Vela Jr.) ● Test supernova explosion theories -> This talk -> M. Renaud (how much 44 Ti do Type Ia SNe (e.g. Tycho) produce?) ● Cassiopeia A: the most certain source of 44 Ti 44 Ti Emission from Cassiopeia A Jacco Vink Estec, Noordwijk, January 19, 2005
Explosive Nucleosynthesis (Kifonidis et al 03) Burrows, astro-ph/0405427 (densities) MHD: formation of jets? Evolution of fast fingers, containing 56 Ni (can escape in Type Ib/c SNe ) 44 Ti Emission from Cassiopeia A Jacco Vink Estec, Noordwijk, January 19, 2005
Page 1 and 2: 44 Ti Emission from Cassiopeia A Ja
Page 3: 44 Ti & Integral IBIS SPI 44 Ti Emi
Page 7 and 8: Detection of 44 Ti emission from Ca
Page 9 and 10: Evidence for Asymmetric Explosion C
Page 11 and 12: What velocities to expect? ● Curr
Page 13 and 14: INTEGRAL Observations Cas A (Amalga
Page 15 and 16: IBIS spectrum Raw spectrum ● 67.9
Page 17: Summary and Conclusions ● 44 Ti a

44Ti Emission from Cassiopeia A - SRON

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