This paper is based on UBVRIJHKLM magnitudes of about 700 O- and B-type stars obtained from the literature. The mean intrinsic colours have been derived with the aid of two-colour diagrams for O- and B-type stars of luminosity classes Ia, Iab–Ib–II, III and IV–V. The present results are based on much larger samples ofevery Sp/L than any other previously determined infrared colours. The colours obtained are compared with those obtained by other authors. In the present system of infrared colours, the intrinsic (B – V)0 values obtained in the programme to determine the intrinsic ultraviolet colours of OB stars (Papaj, Krełowski & Wegner) were used. The majority of slightly reddened Oe and Be stars and all very strongly reddened Be stars adopted in this work are placed on the two-colour diagrams identically as normal B stars. Examples of several two-colour diagrams are presented.
No takes yet. Share an insight, caveat, or question.
W. Wegner (1994) studied this question.