EPJ Web of Conferences
Volume 19, 2012Assembling the Puzzle of the Milky Way
|Number of page(s)||2|
|Section||Disc Non-axisymetries: Spiral, Warp, Bar. What Structure, What Dynamics?|
|Published online||07 February 2012|
The dynamics of long-lived spiral arms
1 Graduate School of Science and Engineering, Kagoshima University, Japan
2 Interactive Research Center of Science, Tokyo Institute of Technology, Japan
3 Division of Theoretical Astronomy, National Astronomical Observatory of Japan, Japan
a e-mail: email@example.com
It has been believed that spiral arms in pure stellar disks decay in several galactic rotations due to the heating by the spiral arms. However, it might be caused by a numerical heating. We performed a three-dimensional N-body simulations with a sufficiently large number of particles and found that stellar disks can maintain spiral arms for more than 10 Gyr without the help of cooling. Spiral arms are transient and recurrent and they heat disk with a heating rate, dQ/dt, correlated to the spiral amplitude |Am|. On the other hand, |Am| is suppressed by Toomre’s Q. Therefore, the dynamical heating becomes less effective in the later phase of the evolution. This mechanism maintain the spiral arms for more than 10 Gyr.
© Owned by the authors, published by EDP Sciences, 2012
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