10.3 Physical Basis
10.3.1 Power Law Relationships
There is no complete physical description of the structure and kinematics
of elliptical galaxies. However, starting from some simple
physical assumptions a rudimentary justification of the method can be 
provided.
Sargent et al. (1977)
pointed out that the assumptions
that all elliptical galaxies have the same surface 
brightness, L 
R2
(Fish 1964) 
and mass-to-light ratio (M/L), together
with the virial theorem relation M 
 R
2, lead to  
the Faber-Jackson relation L 
 
4. These ideas  
were extended by
Djorgovski & Davis
(1987) and
Dressler et
al. (1987b)
who developed the concept of a fundamental plane in the 
3-space of log Ie log Re log 
 where Ie is the 
galaxy surface brightness within the half-light radius,
Re (or diameter Ae).
Combining the results of these three studies,
the equation of the fundamental plane is:
 
 
or expressed in terms of a modified Faber-Jackson relation:
 
  
As Dressler et
al. (1987b)
show, there are only two
independent parameters in the three observables
Ae, Dn, and Ie, so that
Dn / Ae
is a function of  
the normalizing surface brightness only. They find 
Dn / Ae  
The Dn-
 Iex, where x = 0.8. 
This, together with the empirical (Dn-
) relation, 
leads to a formulation of the modified Faber-Jackson relation which is almost
identical to equation (26). Thus the definition of Dn
combines the 
parameters of the fundamental plane in such a way that it 
is viewed edge-on and Dn is therefore a close to
optimal distance indicator. This is illustrated in
Figure 22
which shows the fundamental plane and its projections,
taken from
Faber et al. 1987.
They point out that the existence of the fundamental plane implies 
there are no constraints on the global parameter relations 
for elliptical galaxies other than the Virial Theorem.
This is perhaps the most important difference between the
Dn-
 relation
and the Tully-Fisher methods; the latter, being a single parameter
relationship, requires the action of an extra physical constraint which is 
presumably set during galaxy formation
(Gunn 1988).
Thus the Dn-
relation depends on the physics of galaxy equilibrium rather than 
the physics of galaxy formation.
  
 
  
 
  
 Figure 22. Structural parameters for group galaxies in the 7S
 survey, taken from
 Faber et
 al. (1987).
 (a) log  
 vs log Re; the
 diagonal line of slope -0.5 is the constant mass locus. (b) Surface
 brightness vs log Re, showing the fundamental plane
 almost edge-on. (c) log 
 vs
 surface brightness, showing the fundamental plane nearly face-on; the
 dots show the effect viewing an E3.6 oblate or prolate galaxy seen at
 maximum elongation and as round in projection. (d) log 
 vs (log Re +
 0.84 log Ie) showing the plane exactly edge-on.
relation cannot be justified in terms of a detailed 
physical model such as can be formulated for Type Ia supernovae or
Cepheids. A general physical description has been formulated
using power law relationships
between the structural and kinematic variables that illustrates
the sensitivity of the method to the assumptions.