Introducing PyCross: PyCloudy Rendering Of Shape Software for pseudo 3D ionisation modelling of nebulae

@article{Fitzgerald2020IntroducingPP,
  title={Introducing PyCross: PyCloudy Rendering Of Shape Software for pseudo 3D ionisation modelling of nebulae},
  author={K. Fitzgerald and {\'E} J Harvey and N. Keaveney and Matt Redman},
  journal={Astron. Comput.},
  year={2020},
  volume={32},
  pages={100382}
}
1 Citations
Two new nova shells associated with V4362 Sagittarii and DO Aquilae
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

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Two new nova shells associated with V4362 Sagittarii and DO Aquilae
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
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