Now showing items 1-3 of 3

    • Introducing PyCross: PyCloudy rendering of shape software for pseudo 3D ionisation modelling of nebulae. 

      Fitzgerald, Karol; Harvey, Eamonn J.; Keaveney, Nicola; Redman, Matthew (Elsevier, 2020-04-29)
      Research into the processes of photoionised nebulae plays a significant part in our understanding of stellar evolution. It is extremely difficult to visually represent or model ionised nebula, requiring astronomers to ...
    • Shock shaping? Nebular spectroscopy of nova V906 Carinae 

      Harvey, E.J.; Aydi, E.; Izzo, L.; Morisset, C.; Darnley, M.J.; Fitzgerald, Karol; Molaro, P.; Murphy-Glaysher, F.; Redman, M.P.; Shrestha, M. (Oxford University Press, 2023-03-22)
      V906 Carinae was one of the best observed novae of recent times. It was a prolific dust producer and harboured shocks in the early evolving ejecta outflow. Here, we take a close look at the consequences of these early ...
    • Two new Nova Shells associated with V4362 Sagittarii and DO Aquilae 

      Harvey, E.J.; Redman, M.P.; Boumis, P.; Fitzgearld, Karol; Dulaimi, S.C.; Williams, S.C.; Darnley, M.J.; Lam, M.C.; Kopsacheilli, M.; Derlopa, S. (Oxford Academic, 2020-09)
      A classical nova is an eruption on the surface of a white dwarf in an accreting binary system. The material ejected from the white dwarf surface generally forms an axisymmetric shell. The shaping mechanisms of nova shells ...