Summarized effective temperatures scale of main sequence stars and substars

Abstract

The generalized scale of effective temperatures (T_eff) for substars and main sequence stars in the interval spectral types Sp = O8V ÷ T9,5V. Determined the dependence of effective temperatures T_eff from spectral code C_Sp for Sp = O8V ÷ T9,5V. Approximation executed depending lg T_eff - C_Sp polynomial the fifth power, the relative error free members are less than 17%.

Keywords

• stars
• substars
• scale of effective temperatures