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Vela as the Source of Galactic Cosmic Rays above 100 TeV Abstract: We model the contribution of the nearest young supernova remannt Vela to the local

Vela as the Source of Galactic Cosmic Rays above 100 TeV Abstract: We model the contribution of the nearest young supernova remannt Vela to the local

Co-Production of Light and Heavy p-, s- and r-Process Isotopes in the High-Entropy Wind of Core-Collapse Supernovae doi:10.22323/1.100.008111th

material in Saturns E ring, in which Enceladus ~100 geysers coming from the tiger stripes in //aasnova.org/wp-content/uploads/2015/10/PIA

Primary particle acceleration above 100 TeV in the shell-type Supernova Remnant RX J1713.7-3946 with deep H.E.S.S. observations

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Gamma-Ray Observations of Supernova RemnantsDespite the growing evidence for However, 200 GeV to 100 TeV measurements revealed no significant emission

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Manga- nelli, R., Chan, W.T., Tsenova, L., Gold, B., Smith, P Natl Acad Sci USA 100 : 14321 – 14326

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Abstract: Tychos supernova remnant (SNR) has a periphery which clearly {-1}$, a pole velocity of $\sim 100$~km s$^{-1}$, a duration

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Primary particle acceleration above 100 TeV in the shell-type Supernova Remnant RX J1713.7-3946 with deep H.E.S.S. observations

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