Hi, notknowing,
I agree with George Jones and Pervect (hi, Pervect!) that you must be confusing coordinate speed with physical velocity. You cited the Wikipedia and some website unfamiliar to me, but you appear to have misunderstood something someone said (perhaps taken out of context?), or someone may have misinformed you. If you really want to know anything about gtr, you should obtain a good textbook; gosh knows you have a virtual cornucopia to choose from! I'd recommend Misner, Thorne, and Wheeler, Gravitation, Freeman, 1973 (known as MTW and still widely available), because it probably contains the answer to any answer you might ask.
The basic problem is if you plot some light cones in the Schwarzschild chart outside the event horizon of a nonrotating black hole, they appear to become "radially flattened" and "taller", because the coordinate vectors @/@t, @/@r etc. do not have unit length. If you don't correct for this, you will be incorrectly computing all velocities, including the velocity of a passing laser pulse. If you do correct for this, then of course the speed of light is c=1 (in relativistic or "geometrized" units) everywhere and everywhen, more or less by construction of the theory. (Since our default theory of gravitation is gtr, I assume this is the theory you have in mind.)
As for the quotation from some website which you offered (do you know who wrote it and why they can be considered an "expert"?), it appears that this author may be referring to a distinct issue, that old bugaboo, "local versus global". The clue is that he mentions light bending, which is a curvature effect not seen in an infinitesimally small region.
In the above, I was discussing physics and geometry "at the level of tangent spaces". If you consider "paths" (say of a laser pulse) and "speeds" measured over larger regions of spacetime, you will need to deal with the fact that second order curvature effects will show up. In addition, at the operational level by which we connect our mathematical computations in gtr (our default theory) with what real observers can actually measure, it turns out that there are many distinct notions of "distance in the large" and thus of "velocity in the large". This is a fascinating topic, but not one we should get into unless we are all comfortable with at least the Track One concepts covered in MTW.
You will be interested in an idea put forward long ago by the famous physicist Andrei Sakharov (the same who was a well known political dissident in the former Soviet Union). You can read more about it in Box 17.2 of Misner, Thorne, and Wheeler, Gravitation. I should add that no-one has ever been able to make this work, but it continues to intrigue many physicists.
Chris Hillman