We revisit the problem of collinear solutions of the problem of N bodies, as investigated by Euler and Lagrange. Unlike most existing studies, we consider a general class of attractive forces. In this respect, we follow Newton's attitude in Principia of first con-sidering the problem in its generality, without assuming that the force obeys the gravitational inverse square law. We find that circular concentric orbits, also named relative equilibria, exist as a general fact. Conversely, we show that homographic orbits o exist only for forces that obey a power law.