Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-03-08
Astron.Astrophys.436:607-613,2005
Astronomy and Astrophysics
Astrophysics
7 pages, 11 figures, accepted for publication in A & A
Scientific paper
10.1051/0004-6361:20042432
We present two numerical simulations of an accretion flow from a rotating torus onto a compact object with and without a solid surface -- representing a neutron star and a black hole -- and investigate its influence on the process of jet formation. We report the emergence of an additional ejection component, launched by thermal pressure inside a boundary layer (BL) around the neutron star and examine its structure. Finally, we suggest improvements for future models.
Camenzind Max
Gracia José
Stute Matthias
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