Internal and external shock fronts in He2-104

Abstract

The spectra of both the inner and outer nebulae in He2-104 are modelled by composite models which accounts consistently for photoionisation and shocks. The temperature of the hot star results Ts = 130 000 K. We suggest that the characteristic "crab legs" in He2-104 are produced by R-T instability at the shock front. The calculated X-ray flux is below the detection limit of ROSAT.

MS10595.tex (AA vers.), MS10595f1.jpg, MS10595f2.eps. Accepted for publication in A&A

References in corpus (1)

• Modeling RR Tel through the Evolution of the Spectra

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