COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 1893 Konkoly Observatory Budapest 1980 December 18 HU ISSN 0374-0676 SEARCH FOR AN ECLIPSE OF HR 913 The star HR 913 was discovered by R.F. Griffin (1980) to be a double-lined spectroscopic binary with a period of 363.10 days. Griffin gives the spectral types of the components to be F8 V and G5 V. He predicts the possibility of an eclipse on 1980 September 30.8 (JD 2444513.3) with an uncertainty of 0.5 days. The duration of a central eclipse would also be about half a day. The author searched for the eclipse on four nights with the No. 4 16-inch telescope at Kitt Peak National Observatory. Differential V and B photometric observations were obtained using rho^1 Eri as a comparison star. The observations were corrected fr differential atmospheric extinction and transformed to the standard UBV system. The observations are shown in the Table below. TABLE Hel. J.D. Delta V Delta B (2440000+) 4510.9288 0.443 -0.007 4510.9329 0.441 -0.006 4510.9370 0.438 -0.008 4511.8762 0.442 4511.8793 0.436 4512.8284 0.442 4512.9340 0.446 4513.7986 0.439 4513.9442 0.443 4513.9544 0.447 0.002 4513.9592 0.447 0.000 4513.9937 0.439 -0.005 The data bracket the predicted time of eclipse and show no evidence of an eclipse. However, a 0.5 day eclipse very close to the predicted time would have occurred entirely between the last observation obtained on JD 2444512 and the first observation on JD 2444513 and, hence, would not have been observable from the longitude of Kitt Peak. The author acknowledges that this work was supported in part by N.A.S.A. research grant NSG-7543. GREGORY W. HENRY * Dyer Observatory Vanderbilt University Nashville, Tennessee 37235 Reference: Griffin, R.F., 1980, The Observatory 100,113 [BIBCODE 1980Obs...100..113G ] *Guest Investigator, Kitt Peak National Observatory, which is operated by the Association of Universities for Research in Astronomy, under contract with the National Science Foundation.