Se. Levine et La. Aguilar, THE FUNDAMENTAL PLANE OF ELLIPTIC GALAXIES AND THE VIRIAL-THEOREM, Monthly Notices of the Royal Astronomical Society, 280(2), 1996, pp. 13-17
When an elliptical galaxy undergoes a transformation that satisfies tw
o simple physical assumptions, virial equilibrium and retention of the
functional form of the surface brightness and mass density profiles,
the resulting observable properties of the galaxy lie in a very thin p
arallelepiped in the three-dimensional space defined by effective radi
us, effective surface brightness, and central velocity dispersion, eve
n for large changes in the global mass-to-light ratio (M/L). Additiona
lly, for a fixed M/L, they are quite narrowly constrained in the face
of the parallelepiped. The angle between this plane and the observed F
undamental Plane of elliptical galaxies is less than 15 degrees, imply
ing that most of any predicted change is projected along the Fundament
al Plane, regardless of the specific details of the interaction respon
sible for the change. Tidal interactions are examined as a simple appl
ication.