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Type ii sn - PowerPoint PPT Presentation

Post-Main Sequence Evolution of Massive Stars

Post-Main Sequence Evolution of Massive Stars. Stars of more than 8 solar masses leave behind neutron stars and black holes and typically explode as supernovae. But first, NOVAE from WDs. Back to binary star evolution: More massive star leaves MS first, becomes RG, then WD

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735 views • 45 slides

Near Field Cosmology with Binary ? among extremely metal-poor stars in the Galactic halo??

Near Field Cosmology with Binary ? among extremely metal-poor stars in the Galactic halo??. Yutaka Komiya (Tohoku Univ.) Takuma Suda, Asao Habe, Masayui Fujimoto (Hokkaido Univ.). OMEG07 Hokkaido University Dec. 04, 2007. Near Field Cosmology. ?.

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159 views • 15 slides

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Type ii sn - PowerPoint PPT Presentation

Post-Main Sequence Evolution of Massive Stars

Near Field Cosmology with Binary ? among extremely metal-poor stars in the Galactic halo??