  We study the absorption of massless scalar field by two types furry charged
black holes in de Rham-Gabadadze-Tolley (dRGT) theory. The absorption cross
section is calculated in high frequency limit $\sigma_{hf}$ and low frequency
limit $\sigma_{lf}$. We show that the high frequency limit $\sigma_{hf}$ is the
area of shadow and the low frequency limit $\sigma_{lf}$ is the area of
horizon.
  The ratio $R_{f}=\frac{\sigma_{hf}}{\sigma_{lf}}$ is used to measure the
impact of charges on the absorption spectra of furry black hole. If the black
hole possess an extra charge except mass, the interval value of absorption
ratio $R_{f}$ is different: $[1,\frac{27}{16}]$ for electric charge,
$[0.7675,\frac{27}{16}]$ for positive charge and $[\frac{27}{16},3.1835]$ for
negative charge. We also use a numerical method to compute the absorption cross
section in the finite frequency domain. A series of numerical results are
presented.
