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![]() Date: 2012-04-30 03:30:11Astrophysics Light sources Supernovae Silicon-burning process Star Stellar evolution R-process Supernova Stellar nucleosynthesis Physics Nucleosynthesis Nuclear physics | Add to Reading List |
![]() | “First Lock” Barry Barish 21 October 2000 LIGO is operated by MIT & Caltech for the National Science FoundationDocID: 13HzI - View Document |
![]() | Evolution and nucleosynthesis prior to the AGB phase Amanda Karakas Research School of Astronomy & Astrophysics Mount Stromlo ObservatoryDocID: 10RtT - View Document |
![]() | Lecture 12 Advanced Stages of Stellar Evolution – II Silicon Burning and NSE The solution of reaction networks.DocID: IxqU - View Document |
![]() | PDF DocumentDocID: mriZ - View Document |
![]() | Chapter 11 Pre-supernova evolution of massive starsDocID: 4Rtg - View Document |