Items where Author is "Nomoto, K."

Number of items: 9.
Article
  • Spectroscopic studies of extremely metal-poor stars with the Subaru high dispersion spectrograph. IV : The alpha-element-enhanced metal-poor star BS16934-002. (2007) W. Aoki, S. Honda, T.C. Beers, M. Takada-Hidai, N. Iwamoto, N. Tominaga, H. Umeda, K. Nomoto, J.E. Norris and Sean G. Ryan
  • Nucleosynthetic signatures of the first stars. (2005) A. Frebel, W. Aoki, N. Christlieb, H. Ando, M. Asplund, P.S. Barklem, T.C. Beers, K. Eriksson, C. Fechner, M.Y. Fujimoto, S. Honda, T. Kajino, T. Minezaki, K. Nomoto, J.E. Norris, Sean G. Ryan, M. Takada-Hidai, S. Tsangarides and Y. Yoshii
  • The new record holder for the most iron-poor star: HE 1327−2326, a dwarf or subgiant with [Fe/H] = −5.4. (2005) A. Frebel, W. Aoki, N. Christlieb, H. Ando, M. Asplund, P.S. Barklem, T.C. Beers, K. Eriksson, C. Fechner, M.Y. Fujimoto, S. Honda, T. Kajino, T. Minezaki, K. Nomoto, J.E. Norris, Sean G. Ryan, M. Takada-Hidai, S. Tsangarides and Y. Yoshii
  • Lifetime of Type Ia Supernovae and chemical evolution of Galaxies. (2003) C. Kobayashi and K. Nomoto
  • Nucleosynthesis and stellar evolution. (2002) Friedrich-Karl Thielemann, D. Argast, F. Brachwitz, G. Martinez-Pinedo, T. Rauscher, M. Liebendoerfer, A. Mezzacappa, P. Hoflich and K. Nomoto
  • Other
  • Chemodynamical evolution of the Milky Way. (2003) C. Kobayashi, N. Nakasato and K. Nomoto
  • Type Ia supernovae : Progenitors and diversities. (2003) K. Nomoto, T. Uenishi, C. Kobayashi, H. Umeda, T. Ohkubo, I. Hachisu and M. Kato
  • Nucleosynthesis in supernovae. (2002) Friedrich-Karl Thielemann, D. Argast, F. Brachwitz, Gabriel Martinez-Pinedo, T. Rauscher, M. Liebendoerfer, A. Mezzacappa, P. Hoflich, K. Iwamoto and K. Nomoto
  • Element synthesis in stars. (2001) Friedrich-Karl Thielemann, F. Brachwitz, C. Freiburghaus, E. Kolbe, Gabriel Martinez-Pinedo, T. Rauscher, F. Rembges, W. R. Hix, M. Liebendoerfer, A. Mezzacappa, K.L. Kratz, B. Pfeiffer, K. Langanke, K. Nomoto, S. Rosswog, H. Schatz and Michael Wiescher