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The top documents tagged [accretion disk heats]
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Summary of Post-Main-Sequence Evolution of Sun-Like Stars M < 4 M sun Fusion stops at formation of C,O core. C,O core becomes degenerate Core collapses;
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© 2004 Pearson Education Inc., publishing as Addison-Wesley The Bizarre Stellar Graveyard
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Degenerate Matter and White Dwarfs. Summary of Post-Main-Sequence Evolution of Sun-Like Stars M < 4 M sun Fusion stops at formation of C,O core. C,O core
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Summary of Post-Main-Sequence Evolution of Sun-Like Stars
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Death of Stars I
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Black Holes Accretion Disks X-Ray/Gamma-Ray Binaries
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X-Ray Binaries as Gamma-Ray Sources
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