The answer to this question depends on whether we are dealing with relativistic systems or not. The answer by Arthur refers to the relativistic case where the wavelength changes because of Lorentz contraction. In my opinion the non-relativistic case of Schroedinger waves is rather more interesting because what happens is quite subtle. Suppose we have a solution $\psi(x,t)$ to the Schroedinger equation
$$
i\hbar\frac{\partial \psi}{\partial t} = -\frac {\hbar^2}{2m}
\frac {\partial^2\tilde \psi }{\partial x^2} + V(x)\psi,
$$
and look at it from a moving frame where the equation becomes
$$
i\hbar\frac{\partial \tilde\psi}{\partial t} = -\frac {\hbar^2}{2m}
\frac {\partial^2\tilde \psi }{\partial x^2} + V(x-Ut)\tilde\psi.
$$
Then some manipuations with the chain-rule for partial derivatives shows that we must have
$$
\tilde \psi(x,t)= e^{imUx/\hbar -i\frac 12
mU^2t/\hbar}\psi(x-Ut,t).
$$
The extra phases mean that quantum wavefunctions do not transform as scalars under Galilean transformations. For example the wavefunction for an electron in the ground state of a hydrogen atom is a real function, but seen by someone running at speed $U$ towards the atom, the electron has a net momentum $p=mU$ towards the runner and the wavefunction has an $e^{-imU/\hbar}$ factor.
How this arises is quiate interesting. To get the non-relativistic wavefunction $\psi(x,t)$ for a particle of mass $m$ from a relativistic wavefunction $\phi(x,t)$ that does transform as a scalar, we write
$$
\phi(x,t)= e^{-imc^2 t/\hbar}\psi(x,t).
$$
In other words the non-relativistic $\psi$ does not include the phase coming from the $mc^2$ rest-mass energy.
Suppose now we make a Lorentz transform
$$
x\to x'= (x-Ut)/\sqrt{1-U^2/c^2},
$$
$$
t\to t' = (t+Ux/c^2)/\sqrt{1-U^2/c^2}.
$$
Even when $U$ is very small compared to $c$ --- so that we are effectively making a Galilean transform ---
the $c^2$ in the $mc^2$ cancels with the $c^2$ in the $x/c^2$ term and the result is the extra factor of $e^{imUx/\hbar}$ in $\tilde \psi$.
I first learned all this from a problem at the end of Chapter 22 in Gordon Baym's "Lectures on Quantum Mechanics."