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Astron. Astrophys. 337, 393-402 (1998)

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1. Introduction

For a proper introduction to this paper dealing with the photometric variability of evolved massive stars, the [FORMULA] Cyg variables, we refer the reader to our previous paper (van Genderen et al. 1998, hereafter Paper I). In the present paper we discuss VBLUW photometry (Walraven system) and uvby photometry (Strömgren system) of R 85 and R 110 (two emission-line supergiants and LBVs in the LMC) and VBLUW photometry of the supergiant R 42 and the hypergiant R 45 (both in the SMC).

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© European Southern Observatory (ESO) 1998

Online publication: August 17, 1998
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