Now showing items 1-4 of 4

    • Chemodynamical simulations of the Milky Way Galaxy 

      Kobayashi, Chiaki (Cambridge University Press, 2009)
      We simulate the chemodynamical evolution of the Milky Way Galaxy, including the nucleosynthesis yields of hypernovae and a new progenitor model for Type la Supernovae (SNe la). In our nucleosynthesis yields of core-collapse ...
    • H I in galactic disks 

      Brinks, E.; Bigiel, Frank; Leroy, Adam; Walter, Fabian; de Blok, W. J. G.; Bagetakos, Ioannis; Usero, Antonio; Kennicutt, Robert C. (Cambridge University Press, 2009)
      Studies of the atomic phase of the interstellar medium, via the 21-cm spectral line of neutral hydrogen (H I), play a key role in our attempts to understand the structure and evolution of disk galaxies. We present here ...
    • The Hamburg/ESO R-process Enhanced Star survey (HERES). I : Project description and discovery of two stars with strong enhancements of neutron-capture elements 

      Christlieb, N.; Beers, T.C.; Barklem, P.S.; Bessell, M.S.; Hill, V.; Holmberg, J.; Korn, A.J.; Marsteller, B.; Mashonkina, L.; Qian, Y.Z.; Rossi, S.; Wasserburg, G.J.; Zickgraf, F.J.; Kratz, K.L.; Nordstrom, B.; Pfeiffer, B.; Rhee, J.; Ryan, Sean G. (2004-12)
    • A new sample of extremely/ultra metal-poor stars 

      Perez, A. E. Garcia; Christlieb, N.; Ryan, Sean G.; Beers, T.C.; Aoki, W.; Asplund, M.; Barklem, P.S.; Bessell, M.S.; Eriksson, K.; Frebel, A.; Gustafsson, B.; Korn, A.J.; Nordstrom, B.; Norris, J.E. (2008-12)
      A sample of 30 very metal-poor stars from the Hamburg-European Southern Observatory (ESO) objective-prism survey have been observed at high spectral resolution at the Very Large Telescope (VLT) using the Ultraviolet and ...