Now showing items 1-2 of 2
Introducing PyCross: PyCloudy rendering of shape software for pseudo 3D ionisation modelling of nebulae.
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 ...
Two new Nova Shells associated with V4362 Sagittarii and DO Aquilae
(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 ...