COMMISSION 27 OF THE I.A.U. INFORMATION BULLETIN ON VARIABLE STARS Number 1473 Konkoly Observatory Budapest 1978 September 18 R Pup - A VARIABLE AFTER ALL The G0Ia supergiant R Pup (HD 62058) was first reported by Gould (1879) to be variable. During the following century however its variability could not be confirmed by any of the numerous subsequent observers. R Pup thus was considered constant since 1907 although recently White (1975) finds some possible evidence for very slow variations in both brightness and colours. R Pup was observed in UBV on 7 nights between January 3 and January 30, 1977. The comparison stars used were HD 61409 a K0 star and HD 60646 a F0 star. Their, respective magnitudes remained constant within 0m.002 during this period. R Pup revealed definite variations in magnitude and colours on a time scale well exceeding the 27 days covered by the observations, the V magnitude dropping by about 0m.002 a day towards a minimum. The overall amplitude observed was 0m.19 in U, 0m.12 in B and 0m.06 in V but is certainly larger. The behaviour of R Pup is strikingly similar to that of HD 101947 for which G0Ia star Reipurth and Eichendorf (1978) presume that it may be a very long-period low-amplitude classical cepheid. Observations of that star and of other hitherto unsuspected supergiants will be submitted shortly to Astronomy and Astrophysics. M.J. STIFT Institut fur Astronomie der Universitat Wien Turkenschanzstr. 17 A-1180 Wien, Austria References: Gould, B.A.: 1879, Res. Obs. Nac. Argentino Cordoba, 1 [BIBCODE 1879RNAO....1....0G ] Reipurth, B., Eichendorf, W.: 1978, I.B.V.S. No. 1450 White, S.D.M.: 1975, Astrophys. J. 197, 67 [BIBCODE 1975ApJ...197...67W ]