On the zero point constant of the bolometric correction scale

Arbitrariness attributed to the zero-point constant of the V-band bolometric corrections (BC_V) and its relation to 'bolometric magnitude of a star ought to be brighter than its visual magnitude' and 'bolometric corrections must always be negative' was investigated. The falsehood of the second assertion became noticeable to us after IAU 2015 General Assembly Resolution B2, where the zero-point constant of bolometric magnitude scale was decided to have a definite value C_Bol(W) = 71.197 425 ... . Since the zero-point constant of the BC_V scale could be written as C₂ = C_Bol - C_V, where C_V is the zero-point constant of the visual magnitudes in the basic definition BC_V = M_Bol - M_V = m_bol - m_V, and C_Bol > C_V, the zero-point constant (C₂) of the BC_V scale cannot be arbitrary anymore; rather, it must be a definite positive number obtained from the two definite positive numbers. The two conditions C₂ > 0 and 0 < BC_V < C₂ are also sufficient for L_V < L, a similar case to negative BC_V numbers, which means that 'bolometric corrections are not always negative'. In sum it becomes apparent that the first assertion is misleading causing one to understand bolometric corrections must always be negative, which is not necessarily true.