COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 3543 Konkoly Observatory Budapest 21 November 1990 HU ISSN 0374 - 0676 THE DISCOVERIES OF V154 IN M 3 In March 1899 E. E. Barnard discovered one of the brighter stars very near the center of the globular cluster M3 to be variable, and eventually he published (Barnard 1906) a chart and visual light curve with a period of 15.8 days for it. The star is listed as variable No. 154 in this cluster by Sawyer (1939). This object was considered by Barnard to be new since it was not contained in Bailey's (1902) extensive list of variables in M3, and it has generally been termed Barnard's variable (Greenstein 1935 and Joy 1940, 1949). It is an interesting fact, however, that this star had already been discovered to be variable by E. C. Pickering almost ten years before Barnard's discovery, from four plates taken by the Harvard expedition to Mount Wilson in the summer of 1889, though the announcement (Pickering 1889) did not provide either a chart or light curve. The variability of this important object, which is the first pulsating variable to be discovered in any globular cluster, was thus a Harvard discovery, though its nature was first recognized at Yerkes. WILLIAM P. BIDELMAN Warner and Swasey Observatory Case Western Reserve University Cleveland, OH 44106 References: Bailey, S.I. 1902, Harvard Ann., 38, 238. [BIBCODE 1902AnHar..38....1B ] Barnard, E.E. 1906, Astr. Nach., 172, 345. [BIBCODE 1906AN....172..345B ] Greenstein, J.L. 1935, Harvard Bull., 901, 11. [BIBCODE 1935BHarO.901...11G ] Joy, A.H. 1940, Ap. J., 92, 396. [BIBCODE 1940ApJ....92..396J ] --------- 1949, Ap. J., 110,105. [BIBCODE 1949ApJ...110..105J ] Pickering, E.C. 1889, Astr. Nach., 123, 207. Also see Harvard Ann., 38, 1, 1902. [BIBCODE 1889AN....123..207P ] Sawyer, H.B. 1939, Publ. David Dunlap Obs., 1, 150. [BIBCODE 1939PDDO....1..125S ]