'Emp stars' diaporamas de présentation

Contents

Pop III Black-hole-forming supernovae and Abundance pattern of Extremely Metal Poor Stars Hideyuki Umeda ( ???? ) Dept. of Astronomy Univ.of Tokyo work with Prof.K. Nomoto. Contents. Can Core-collapse Supernova yields explain the abundance pattern of

472 views • 37 slides

The 0Z Project

The 0Z Project. The core group: Judy Cohen (Caltech), Andy McWilliam, Steve Shectman, Ian Thompson (Carnegie), Norbert Christlieb (Hamburg) Current and former postdocs: Inese Ivans, Jorge Melendez, Solange Ramirez (Caltech), Innocenza Busa, Franz-Josef Zickgraf (Hamburg)

391 views • 32 slides

Nucleosynthesis in Population III Supernovae and Abundance Patterns of Hyper Metal-Poor Stars

Nucleosynthesis in Population III Supernovae and Abundance Patterns of Hyper Metal-Poor Stars. N. Tominaga, H. Umeda, K. Maeda, K. Nomoto (Univ. of Tokyo), N. Iwamoto (JAERI). Contents. Hyper Metal-Poor stars Supernovae of Population III stars

451 views • 28 slides

Nucleosynthesis in Population III Supernovae and Abundance Patterns of Hyper Metal-Poor Stars

Nucleosynthesis in Population III Supernovae and Abundance Patterns of Hyper Metal-Poor Stars. N. Tominaga, H. Umeda, K. Maeda, K. Nomoto (Univ. of Tokyo), N. Iwamoto (JAERI). Contents. Hyper Metal-Poor stars Supernovae of Population III stars

282 views • 28 slides

Nucleosynthesis in Pop III, Massive and Low-Mass Stars

311 views • 19 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. ?.

159 views • 15 slides

Supernova Nucleosynthesis and Extremely Metal-Poor Stars

Supernova Nucleosynthesis and Extremely Metal-Poor Stars. Nozomu Tominaga (Univ. of Tokyo). Collaborators: H.Umeda, K.Maeda, N.Iwamoto, K.Nomoto. OMEG07, 4-7 Dec. 2007, Hokkaido Univ. Core-Collapse SNe. Core collapse Compact object n emission Energy deposition. Massive Star (>10M 8 )

136 views • 13 slides