4. Spiral galaxies (Françoise Combes)
The FILM (mpg, 65 Mb; gif, 5,1 Mb) shows separately stars LEFT and gas RIGHT.
It shows how, starting from an initially relatively homogeneous state (flat disk with axial symmetry), the gaz clouds and stars moving along their orbits generate instabilitiess which lead to spiral arms.
Stars form only transient spirals, because instabilities heat them, which stops the instability.
The bar in the center is robust however (there is no gravitational couple from the bar on itself, because the potential is in phase with the density, which is not the case of the spiral arms).
The gas is dissipative, cools and is always unstable, so it forms spirals again and again.
Lindblad's resonance (ring formation) is the same as the one which gives rise to Saturn's rings. The resonance occurs between the movements of the stars (or of the clouds) and that of the perturbation (bar or spiral): when the frequencies are in a rational ratio.
There are in general two arms in a galaxy, so the relevant
resonances are: Omegab = Omega-kappa/2 et externe Omegab=Omega+kappa/2
(Omega is the frequency of the star's rotation, Omegab
is the frequency of rotation of the bar, kappa: epicyclic frequency)