$A$ Cassegrain telescope uses two mirrors of radii of curvature $25 \ cm$ and $16 \ cm$ separated by a distance of $2.5 \ cm$. The position of the final image of an object at infinity is

  • A
    $40 \ cm$ from convex mirror
  • B
    $4.44 \ cm$ from concave mirror
  • C
    $4.44 \ cm$ from convex mirror
  • D
    $40 \ cm$ from concave mirror

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