Astronomy and Astrophysics – Astrophysics
Scientific paper
1997-01-17
Astronomy and Astrophysics
Astrophysics
14 pages, aasms4.sty, 3 figures not included (available upon request) To appear in ApJ Letters. email chy, jhh@crater.nju.edu.
Scientific paper
10.1086/310582
We find that a non-axisymmetric bow shock model, with an appropriate choice of parameters, could fit the line splitting velocity field of the cone-like H$\alpha$ nebula in NGC 4945 better than a canonical cone model. Meanwhile, the bow shock model could also reproduce the morphology of the H$\alpha$ nebula. The bow shock results from the interaction of the galactic superwinds with a giant HII region. It is implied that the starburst ring or disk around the galactic nucleus should be generating strong winds, and the bright H$\alpha$ knot northwest of the nucleus be suffering an anisotropic mass loss process.
Chen Yang
Huang Jie-Hao
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