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phy232topic1.ppt
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A search for supernovae in galaxy clusters at 0.1 < z < 0.2 David J Sand (U of A) Chandra Fellows Symposium 2007 See arXiv0709.2519
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Black holes: Introduction. 2 NS to BH 1209.0783 The authors studied collapse from NS to BH. Calculations were done for two cases: with and without massive
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PAMELA measurements of proton and helium nuclei and cosmic ray acceleration in the galaxy M. Casolino RIKEN – ASI INFN & University of Rome Tor Vergata
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Inma Domínguez Explosive Nucleosynthesis in Type Ia Supernovae Universidad de Granada Dust in EuroGENESIS environments: from primitive, massive stars to
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Supernovae and Masers in Arp220: Pushing the limits of VLBI sensitivity
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