This is accounted for in real models of the rotation curves of galaxies. The rotation curve of a galaxy is more complicated than the motion of planets in the solar system, for the reasons that you describe.
A trivial model would consider the galaxy as spherically symmetric and would use the shell theorem to estimate the centripetal acceleration of a star at radius r. Thus
mromega2=GfracmM(r)r2,
where m is the mass of the star, omega is the angular velocity and M(r) would be the mass of all gravitating matter at radii <r. Note that this only applies to a spherically symmetric distribution of mass.
To make further progress demands that you know the density distribution of the gravitating matter. Let's just assume that density rho is constant for the moment. Then
r3omega2=Gintrho4pir2dr=frac4pi3Grhor3
omega=sqrtfrac4piGrho3
Thus the angular velocity would be constant with radius and the rotation speed, v=omegar would increase with radius. This I think is the situation that your question supposes and so yes, if there was a constant (or perhaps slowly declining) density of material in the Galaxy then this would produce a rotation curve that increased (or was flat).
The trouble is that the density of material in our Galaxy inferred from the matter that we can see is not constant with radius. It declines rapidly and exponentially, such that there is very little visible matter beyond a radius of about 15 kpc. If we take a situation where we go to radii beyond the gravitating matter, then a similar treatment to the above suggests that
mromega2=GfracmMr2,
where M is now the total mass of the (visible) Galaxy. In this case
omega=sqrtfracGMr3
and the rotation velocity v=omegar should decline as 1/sqrtr (like it does in the solar system).
It is the fact that the rotation velocity of stars and gas at large radii (>15 kpc) continues to be flat or even increase that leads to the conclusion that the mass that we can see is not all that there is. i.e That we need "dark matter" to explain the high rotation speeds at radii where there is very little visible matter.
Realistic models of the galaxy do not make the assumption that the visible matter is spherically symmetric (it isn't). But the conclusions I qualitatively set out above hold in the same way.
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