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The surface brightness radial profiles of disk galaxies are usually modelled
as the sum of a bulge and a disk component. The resulting bulge+disk profile
can in general be written as
|
(32) |
where quantities subscripted with and refer to the bulge and disk
component, respectively. The total brightness predicted by this profile is
|
(33) |
The relative importance of the bulge and disk component in terms of the
brightness they contribute to the overall profile can be quantified by the
bulge/disk ratio , which, from Equations 22 and
28, can be expressed in terms of the bulge and disk parameters as
|
(34) |
where
|
(35) |
is related to the more frequently used bulge/bulge+disk ratio
by the
|
(36) |
The relation between the radii and and the effective
radius of the bulge+disk profile , can be determined using
Equations 18 and 19, whose combination yields
|
(37) |
which, after trivial modifications, becomes
|
(38) |
When values for the ratios and are assumed,
Equation 38 can be solved numerically to obtain the corresponding
values of the ratios
and
.
Numerical values of the latter two ratios are given in Table 7
for some values of the former two.
Now, the general bulge+disk profile can be written as
|
(39) |
In much the same way as Equation 38, Equation 39
can be numerically solved with respect to the ratios
and
if values of
the ratios and are assumed.
Numerical values of the two former ratios are given in Table 8
for the same values of the latter two as in Table 7.
Tables 7 and 8, combined with
Equation 39, allows to write the appropriate bulge+disk profile
for different values of and .
The total brightness predicted by the law can then be written in terms of the
bulge+disk quantities and
as
|
(40) |
and, proceeding like for the pure bulge and disk profiles,
can
be written as
|
(41) |
Values of are given in Table 9.
Next: Bibliography
Up: A. Galaxy Surface Brightness
Previous: A..3 Disk Profile
Mattia Vaccari
2002-01-31