Filip said:
I meant the rate that you would have if you did not have this new velocity.
That still doesn't quite address the issue I think Simon Bridge was raising. Let me re-state what I think you mean in a way that I think addresses it.
For simplicity, let's suppose that the object is not the Sun but a pulsar, so that we have a definite timing signal--the pulsar's pulses of radio waves--that defines the "rate" we are observing. Suppose that you start out at rest relative to the pulsar, and you observe one pulse arriving per second, by your clock.
Now suppose you start moving towards the pulsar at 0.6c. (You'll see in a moment why I picked that velocity.) You will now observe two pulses arriving per second, by your clock. Why? Because of the relativistic Doppler effect. The general formula for the Doppler factor (the ratio of the "rate" you observe while moving relative to the source, to the "rate" you observe when at rest relative to the source) for velocity ##v## (note that this only holds if you are moving directly toward or directly away from the source) is
$$
\frac{\omega}{\omega_0} = \sqrt{\frac{1 + v}{1 - v}}
$$
(in units where ##c = 1##). As you can see, if you plug in ##v = 0.6##, you get a Doppler factor of ##2##.
Note that I made the key qualification, that we are comparing the rate you observe while you are moving relative to the source, with the rate you observe while you are at rest relative to the source. In other words, it's not just "velocity" per se, but specifically velocity relative to the source, that counts.