COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2325 Konkoly Observatory Budapest 2 May 1983 HU ISSN 0374 - 0676 BD +37d443 : A NEW RED VARIABLE STAR BD +37d443 was used as comparison star in the observations of the O-subdwarf BD +37d442 by Bartolini et al. (1982), who accidentally interchanged the identification of the two stars (Rebeirot, 1982). In 1977 BD +37d443 was much fainter than BD +37d442 and BD +37d446, while according to the BD catalogue and for BD +37d442 also from the AGK2 catalogue it was listed as being brighter. On January 6, 1983 BD +37d443 was observed photoelectrically with the 152 cm telescope of Bologna Observatory equipped with a five colour photometer described by Lolli (1983) and resulted as bright as in the BD map. The following differences of magnitude between BD +37.443d and BD +37d442 (that according to Landolt (1973) and Bartolini et al. (1982) presents variations not larger than 0.08m) have been obtained so far: JD-2440000 DeltaV DeltaB Telescope 3454.42 0.58 1.81 60 cm 3458.48 0.63 1.77 60 cm 3483.41 0.58 1.79 60 cm 3495.37 0.55 1.75 60 cm 5341.40 -0.29 1.10 152 cm The spectral type K 0 III published by Rebeirot (1970) suggests that BD +37d443 could be a long period or a semiregular variable star. M. LOLLI L. OCULI A. PICCIONI R. SERRA Dipartimento di Astronomia Dell Universita di Bologna References : Bartolini, C., Bonifazi, A., D'Antona, F., Fusi Pecci, F., Oculi, L., Piccioni, A.: 1982; Astrophys. Space Science 83, 287 [BIBCODE 1982Ap&SS..83..287B ] Landolt, A.U.: 1973, Publ. Astron. Soc. Pacific 85, 661 [BIBCODE 1973PASP...85..661L ] Lolli, M.: 1983, Thesis Bologna University Rebeirot, E.: 1970, Astron. Astrophys. 4, 404 [BIBCODE 1970A&A.....4..404R ] Rebeirot, E.: 1982, Astrophys. Space Science 88, 253 [BIBCODE 1982Ap&SS..88..253R ]