As the magnification increases to the field of view decreases, which reduces the amount of light making the image.A 12” telescope gathers more light than a 6” telescope, and has greater resolution no matter what eyepiece you use.
Light gathering and resolution are invariant.
The image gets dimmer as the magnification is increased, but the instrument does not gather less light.
Where a telescope has a primary folal length of say 650mm and a 130mm diameter tube it will have an aperture value of f/5, and this will be printed on the side or in the spec sheet.
Where another telescope has a focal length of say 1300mm in the same 130mm diameter tube, it will have an aperture value of f/10, and again will be in its spec sheet.
Where we add an eyepiece (ocular) that will alter the magnification and hence the overall focal length, and again reduce the field of view, and the aperture value.
Do not confuse the iris diameter (objective size) with the aperture value. Although they are often used interchangeably in conversation they mean different things. The former is a diameter measurement, the aperture is dimensionless ratio. The f-number is a measure of how much light passes through the instrument from subject to image. The aperture f-number is /defined/ as focal length divided by iris diameter (the iris is usually the objective). That means a short FL but narrow instrument can have the same f-number as a long FL but wide one e.g. 100/25 = f/4, 200/50 = f/4
If you don't believe me then believe Nikon. They gave the formulae in the links above. You can easily rearrange the equations and work this out.