Intrinsic colour indices of OB supergiants, giants and dwarfs in the UB VRIJHKLM system

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Abstract

This paper is based on UB VRIJHKLM 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 la, Iab-Ib-II, III and IV-V. The present results are based on much larger samples of every 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, Kretowski & 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.

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Wegner, W. (1994). Intrinsic colour indices of OB supergiants, giants and dwarfs in the UB VRIJHKLM system. Monthly Notices of the Royal Astronomical Society, 270(2), 229–234. https://doi.org/10.1093/mnras/270.2.229

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