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A..4 Bulge+Disk Profile

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

\begin{displaymath}\begin{split}\Sigma_{b+d}(r)&=\Sigma_b(r) + \Sigma_d(r)=\\ &=...
...,e}\,\exp \left(-1.6783\,\frac{r}{r_{d,e}}\right)~, \end{split}\end{displaymath} (32)

where quantities subscripted with $ b$ and $ d$ refer to the bulge and disk component, respectively. The total brightness predicted by this profile is

$\displaystyle F_{b+d,tot}=F_{b,tot}+F_{d,tot}=22.665\,\Sigma_{b,e}\,r_{b,e}^2+ 11.948\,\Sigma_{d,e}\,r_{d,e}^2~.$ (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 $ B/D$, which, from Equations 22 and 28, can be expressed in terms of the bulge and disk parameters as

$\displaystyle \frac{B}{D}=\frac{k_4\,\Sigma_{b,e}\,r_{b,e}^2}{k_1\,\Sigma_{d,e}...
...}{\Sigma_{d,e}} \,\frac{r_{b,e}^2}{r_{d,e}^2}=1.8969\,\rho_{\Sigma}\,\rho_r^2~,$ (34)

where

$\displaystyle \rho_{\Sigma}=\frac{\Sigma_{b,e}}{\Sigma_{d_e}}~,~~~~~~~~ \rho_r=\frac{r_{b,e}}{r_{d,e}}~.$ (35)

$ B/D$ is related to the more frequently used bulge/bulge+disk ratio $ B/T$ by the

$\displaystyle \frac{B}{D} = \frac{B/T}{1-B/T}~.$ (36)

The relation between the radii $ r_{b,e}$ and $ r_{d,e}$ and the effective radius of the bulge+disk profile $ r_{b+d,e}$, can be determined using Equations 18 and 19, whose combination yields

$\displaystyle \frac{k_4}{\Gamma(8)}\,\Sigma_{b,e}\,r_{b,e}^2\,\gamma\left(8\, ,...
...frac{k_4}{2}\,\Sigma_{b,e}\,r_{b,e}^2+ \frac{k_1}{2}\,\Sigma_{d,e}\,r_{d,e}^2~,$ (37)

which, after trivial modifications, becomes

$\displaystyle \frac{B}{D}\,\left[\frac{1}{\Gamma(8)}\, \gamma\left(8\, , \,b_4\...
...t(2\, , \,b_1\,\rho_r\,\frac{r_{b+d,e}}{r_{b,e}}\right) -\frac{1}{2}\right]=0~.$ (38)

When values for the ratios $ B/D$ and $ \rho_r$ are assumed, Equation 38 can be solved numerically to obtain the corresponding values of the ratios $ r_{b,e}/r_{b+d,e}$ and $ r_{d,e}/r_{b+d,e}$. Numerical values of the latter two ratios are given in Table 7 for some values of the former two.

Table 7: Values of $ r_{b,e}/r_{b+d,e}$ and $ r_{d,e}/r_{b+d,e}$ for some values of $ B/D$ and $ \rho_r$. Values calculated via Newton integration (see Section 9.7 in [Press et al.(1992)]) of Equation 38.
$ \frac{r_{b,e}}{r_{b+d,e}}$   $ B/D$
    0.333 0.444 0.555 0.666 0.777
$ \rho_r$ 0.3 0.37776903 0.39659331 0.41501285 0.43296121 0.45038387
  0.4 0.47738606 0.49489417 0.51165418 0.52767183 0.54296003
  0.5 0.57169562 0.58717625 0.60178337 0.61556793 0.62857967
  0.6 0.66216968 0.67514232 0.68725805 0.69858888 0.70920016
  0.7 0.74977666 0.75987986 0.76924321 0.77794075 0.78603748
$ \frac{r_{d,e}}{r_{b+d,e}}$   $ B/D$
    0.333 0.444 0.555 0.666 0.777
$ \rho_r$ 0.3 1.2592301  1.3219777  1.3833761  1.4432040  1.5012795 
  0.4 1.1934651  1.2372354  1.2791355  1.3191796  1.3574001 
  0.5 1.1433912  1.1743525  1.2035667  1.2311359  1.2571593 
  0.6 1.1036161  1.1252372  1.1454301  1.1643148  1.1820002 
  0.7 1.0711095  1.0855427  1.0989189  1.1113440  1.1229107 

Now, the general bulge+disk profile can be written as

\begin{displaymath}\begin{split}\Sigma_{b+d}(r)&=\frac{\Sigma_{b,e}}{\Sigma_{b+d...
...c{r_{b+d,e}}{r_{d,e}}\,\frac{r}{r_{b+d,e}}\right)~. \end{split}\end{displaymath} (39)

In much the same way as Equation 38, Equation 39 can be numerically solved with respect to the ratios $ \Sigma_{b,e}/\Sigma_{b+d,e}$ and $ \Sigma_{d,e}/\Sigma_{b+d,e}$ if values of the ratios $ B/D$ and $ \rho_r$ 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.

Table 8: Values of $ \Sigma_{b,e}/\Sigma_{b+d,e}$ and $ \Sigma_{d,e}/\Sigma_{b+d,e}$ for the same values of $ B/D$ and $ \rho_r$ as in Table 7. Values calculated from Equations 32 and 34, and from Table 7.
$ \frac{\Sigma_{b,e}}{\Sigma_{b+d,e}}$   $ B/D$
    0.333 0.444 0.555 0.666 0.777
$ \rho_r$ 0.3 1.5059000  1.6695642  1.7862309  1.8669555  1.9202392 
  0.4 0.90250402 1.0169289  1.1059437  1.1750876  1.2286100 
  0.5 0.61171687 0.69840479 0.76930751 0.82759966 0.87573973
  0.6 0.44733235 0.51643686 0.57490397 0.62470279 0.66737834
  0.7 0.34431760 0.40137789 0.45089086 0.49413744 0.53213802
$ \frac{\Sigma_{d,e}}{\Sigma_{b+d,e}}$   $ B/D$
    0.333 0.444 0.555 0.666 0.777
$ \rho_r$ 0.3 0.57903215 0.51357003 0.45788132 0.41020644 0.36917465
  0.4 0.61692617 0.55611501 0.50399454 0.45900376 0.41992150
  0.5 0.65336297 0.59676211 0.54778829 0.50511037 0.46768035
  0.6 0.68801330 0.63543886 0.58948209 0.54903740 0.51322600
  0.7 0.72080756 0.67220776 0.62927470 0.59111205 0.55699899

Tables 7 and 8, combined with Equation 39, allows to write the appropriate bulge+disk profile for different values of $ B/D$ and $ \rho_r$. The total brightness predicted by the law can then be written in terms of the bulge+disk quantities $ r_{b+d,e}$ and $ \Sigma_{b+d,e}$ as

$\displaystyle F_{D,tot}=\left[k_4\,\frac{\Sigma_{b,e}}{\Sigma_{b+d,e}} \,\left(...
...ght]\,\Sigma_{b+d,e}\,r_{b+d,e}^2 \equiv k_{b+d}\,\Sigma_{b+d,e}\,r_{b+d,e}^2~,$ (40)

and, proceeding like for the pure bulge and disk profiles, $ \mu_{b+d,e}$ can be written as

$\displaystyle \mu_{b+d,e}=\,2.5\,\log(k_{b+d})+5\,\log(r_{e,\mathrm{[as]}})+ I_{\mathrm{[mag]}}~~~\mathrm{[mag~arcsec^{-2}]}~.$ (41)

Values of $ k_{b,d}$ are given in Table 9.

Table 9: Values of $ k_{b+d}$ for the same values of $ B/D$ and $ \rho_r$ as in Tables 7 and 8. Values calculated from Equation 40 and from Tables 6, 7 and 8.
$ k_{b+d}$   $ B/D$
    0.333 0.444 0.555 0.666 0.777
$ \rho_r$ 0.3 15.841388  16.675985  17.443019  18.140889  18.770256 
  0.4 15.161182  15.816591  16.415234  16.959955  17.454163 
  0.5 14.737528  15.291208  15.795789  16.255446  16.674198 
  0.6 14.458169  14.948771  15.395577  15.803140  16.175547 
  0.7 14.268144  14.717733  15.127242  15.501275  15.843825 


next up previous
Next: Bibliography Up: A. Galaxy Surface Brightness Previous: A..3 Disk Profile
Mattia Vaccari 2002-01-31