In the Johnson → UBV system, a reddening-free parameter which is related to the
→ effective temperature of stars and thus provides a useful, but rough, discriminant for → spectral types. It is expressed as: Q = (U - B) - 0.72 (B - V).
In the Johnson → UBV system, a reddening-free parameter which is related to the
→ effective temperature of stars and thus provides a useful, but rough, discriminant for → spectral types. It is expressed as: Q = (U - B) - 0.72 (B - V).