Stellar cores - PowerPoint PPT Presentation

Gravitational collapse of stellar cores and Supernovae (neutrino fluxes and shock waves)

Gravitational collapse of stellar cores and Supernovae (neutrino fluxes and shock waves). D.K. Nadyozhin. Institute for Theoretical and Experimental Physics ITEP, Moscow, Russia. 23rd European Cosmic Ray Symposium Moscow, Russia, July, 3 - 7 , 2012.

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White Dwarf Stars

White Dwarf Stars. Low mass stars are unable to reach high enough temperatures to ignite elements heavier than carbon in their core become white dwarfs. Hot exposed core of an evolved low mass star.

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1.01k views • 10 slides

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