COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2034 Konkoly Observatory Budapest 1981 November 3 HU ISSN 0374-0676 BD-8d4232, A NEW DELTA SCUTI STAR? In the course of a programme of photometry of hot hydrogen-deficient stars (or helium stars) using the 1m telescope of the South African Astronomical Observatory, BD-8d4232 and BD-9d4385 (= HD148021) were used as comparisons for the helium star BD-9d4395. Figure 1 shows V-magnitudes (colour-corrected from observations through a Stromgren "y" filter) for the two comparison stars during a short run made on 1981 Jun 28/29. BD-8d4232 [FIGURE 1] appears to vary with an amplitude of 0.03 and a period probably ~0.1d. The slight dip in the magnitude of BD-9d4385 after H.J.D. 244 4784.48 is caused by s transparency deterioration rather than intrinsic stellar variability. Table I Stromgren colours for BD-8d4232 HJD V (b-y) M_1 C_1 --------------------------------------------- 2444782.374 9.681 0.352 0.143 0.952 4784.350 9.682 0.354 0.147 0.934 4822.237 9.695 0.359 0.138 0.954 .256 9.681 0.364 0.131 0.947 .370 9.677 0.375 0.121 0.940 4823.245 9.674 0.355 0.131 0.965 .306 9.676 0.358 0.140 0.939 .340 9.670 0.363 0.143 0.906 Stromgren photometry of BD-8d4232 is given in Table I. The (b-y) and C_1 indices indicate a reddening E(b-y) = 0.275 and a spectral type around A7 (cf. Crawford 1979; Table 2). The Smithsonian Star Catalogue gives a spectral type of A5. The short time scale of variation and the spectral type of BD-8d4232 suggest that it is a Delta Scuti type variable (cf. Baglin et.al. 1973). DAVID KILKENNY South African Astronomical Observatory P O Box 9 Observatory 7935 South Africa References: Baglin, A., Breger, M., Chevalier, C., Hauck, B., le Contel, J.M., Sareyan, J.P. & Valtier, J.C., 1973. Astron. Astrophys. 23, 221. [BIBCODE 1973A&A....23..221B ] Crawford, D.L., 1979. Astron. J., 84, 1858. [BIBCODE 1979AJ.....84.1858C ]