Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...211.1312m&link_type=abstract
American Astronomical Society, AAS Meeting #211, #13.12; Bulletin of the American Astronomical Society, Vol. 39, p.756
Astronomy and Astrophysics
Astronomy
Scientific paper
A previous work by Higdon & Wallin (2003 ApJ, 535, 281: HW) has demonstrated by means of numerical simulations that the optical jets detected in NGC 1097 are consistent with having been formed by a minor-merger. However, this work neglected a significant bar component in the disk which could affect this conclusion. In this work we reproduce the results of HW and then continue further by including a bar component in the disk estimated from K-band observations. Through additional simulations we investigate the overall effect on the jets and whether inclusion of the bar strengthens or weakens support for the minor-merger interpretation.
Heller Clayton
Morris Alfred
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