| Abstract
| - We present an analysis of 555 high-dispersion echelle spectra of 19 Mon obtained from two sites as well as 115 Strömgren uvby observations. We show that three periodicities are present at 5.229 94, 0.170 19 and 4.889 56 cycle d−1. The first periodicity has by far the largest amplitude. Photometric amplitude ratios and phase differences indicate an ℓ=2 mode, while the line profile variations unequivocally point to ℓ=2,m=-2. Because of the low amplitudes of the other two modes, very little can be said concerning them. Although 19 Mon was originally selected on the basis of its classification as a marginal Be star, the Be nature of the star is not supported by our observations.
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