摘要: Recent, and older accurate, data on (limb-darkened) angular diameters is compiled for 221 stars, as well BV RIJK[12][25] magnitudes those objects, when available. Nine stars (all M-giants or supergiants) showing excess in the [12 25] colour are excluded analysis this may indicate present of dust influencing o ptical near-infrared colours well. Based large sample, Baade-Wesselink surface-brightness (SB) relations presented dwarfs, giants, supergiants dwarfs optical near-infrared. found to follow different SB-relations from non-M particular V -(V R). � ± ��