Degenerate Matter and White Dwarfs Summary of Post-Main-Sequence Evolution of Sun-Like Stars M < 4 Msun Fusion stops at formation of C,O core. 0 C,O core becomes degenerate…
Death of Stars I Physics 113 Goderya Chapter(s): 13 Learning Outcomes: The End of a Star’s Life When all the nuclear fuel in a star is used up, gravity will win over pressure…
Modeling the Spectral Energy Distributions and Variability of BL Lacertae in 2000 Black Holes Accretion Disks X-Ray/Gamma-Ray Binaries Black Holes Just like white dwarfs…
X-Ray Binaries as Gamma-Ray Sources Binary systems of a compact object (neutron star or black hole) and a stellar companion 0 Matter is flowing over from the stellar companion…
Slide 1Summary 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; outer shells…