Now showing items 1-2 of 2

    • Bar evolution over the last 8 billion years: A constant fraction of strong bars in th GEMS Survey 

      Jogee, S.; Barazza, F.D.; Rix, H-W.; Shlosman, I.; Barden, M.; Wolf, C.; Davies, J.; Heyer, I.; Beckwith, S.; Bell, E.F.; Caldwell, J.A.R.; Conselice, J.; Dahlen, T.; Haussler, B.; Heymans, C.; Jahnke, K.; Knapen, J.; Laine, S.; Lubell, G.M.; Mobasher, B.; McIntosh, D.; Meisenheimar, K.; Peng, C.Y.; Sanchez, S.F.; Somerville, R.S.; Wisotzki, L. (2004-11)
      One-third of present-day spirals host optically visible strong bars that drive their dynamical evolution. However, the fundamental question of how bars evolve over cosmological times has yet to be resolved, and even the ...
    • A surprising consistency between the far-infrared galaxy luminosity functions of the field and Coma 

      Hickinbottom, S.; Simpson, C.J.; James, P.A.; Ibar, E.; Carter, D.; Boselli, A.; Collins, C.A.; Davies, J.I.; Dunne, L.; Eales, S.; Fuller, C.; Mobasher, B.; Peletier, R.F.; Phillipps, S.; Smith, Daniel; Smith, R.J.; Valentijn, E.A. (2014-08-01)
      We present new deep images of the Coma Cluster from the ESA Herschel Space Observatory at wavelengths of 70, 100 and 160 μm, covering an area of 1.75 × 1.0 square degrees encompassing the core and south-west infall region. ...