Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-06-21
Astronomy and Astrophysics
Astrophysics
MS10595.tex (AA vers.), MS10595f1.jpg, MS10595f2.eps. Accepted for publication in A&A
Scientific paper
10.1051/0004-6361:20010865
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.
Contini Marcella
Formiggini Liliana
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