Now showing items 1-4 of 4

    • Protoplanetary disc evolution affected by star-disc interactions in young stellar clusters 

      Rosotti, G.~P.; de Juan Ovelar, M.; Hubber, D.~A.; Kruijssen, J.~M.~D.; Ercolano, B.; Walch, S.; Dale, James (2014-07-01)
      Most stars form in a clustered environment. Therefore, it is important to assess how this environment influences the evolution of protoplanetary discs around young stars. In turn, this affects their ability to produce ...
    • Soft X-ray absorption excess in gamma-ray burst afterglow spectra: Absorption by turbulent ISM 

      Tanga, M.; Schady, P.; Gatto, A.; Greiner, J.; Krause, M.~G.~H.; Diehl, R.; Savaglio, S.; Walch, S. (2016-11-01)
      Two-thirds of long duration gamma-ray bursts (GRBs) show soft X-ray absorption in excess of the Milky Way. The column densities of metals inferred from UV and optical spectra differ from those derived from soft X-ray ...
    • STARBENCH: the D-type expansion of an H II region 

      Bisbas, T.~G.; Haworth, T.~J.; Williams, R.~J.~R.; Mackey, J.; Tremblin, P.; Raga, A.~C.; Arthur, S.~J.; Baczynski, C.; Frostholm, T.; Geen, S.; Haugbølle, T.; Hubber, D.; Iliev, I.~T.; Kuiper, R.; Rosdahl, J.; Sullivan, D.; Walch, S.; Wünsch, R.; Dale, James (2015-10-21)
      STARBENCH is a project focused on benchmarking and validating different star formation and stellar feedback codes. In this first STARBENCH paper we perform a comparison study of the D-type expansion of an H II region. The ...
    • Supernova 2006aj and the associated X-Ray Flash 060218 

      Sollerman, J.; Jaunsen, A.O.; Fynbo, J.; Hjorth, J.; Jakobsson, P.; Stritzinger, M.; Feron, C.; Laursen, P.; Ovaldsen, J-E.; Selj, J.; Thone, C.C.; Xu, D.; Davis, T.M.; Gorosabel, J.; Watson, D.; Duro, R.; Ilyin, I.; Jensen, B.L.; Lysfjord, N.; Marquart, T.; Nielsen, T.B.; Naranen, J.; Schwarz, H.E.; Walch, S.; Wold, M.; Ostlin, G. (2006)