Photoevaporating Flows from the Cometary Knots in the Helix Nebula (NGC 7293)
We explain the Hα emission of the cometary knots in the Helix Nebula (NGC 7293) with an analytical model that describes the emission of the head of the globules as a photoevaporated flow produced by the incident ionizing radiation of the central star. We compare these models with the Hα emission obtained from the Hubble Space Telescope (HST)
López-Martín, L. et al.
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2001