COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2880 Konkoly Observatory Budapest 17 March 1986 HU ISSN 0374 - 0676 THE HISTORICAL OPTICAL VARIATION OF DO Dra (=3A1148+719) A search of the Harvard College Observatory plate collection for outbursts of this CV encompassed the following numbers of plates and epochs (all magnitudes are blue): 1) very-wide-angle patrol series: 223 plates with limiting magnitudes of 13.7 mag or fainter, and more than 200 additional plates of limit 12.2 mag or fainter, 1899- 1951; 2) wide-angle patrol series: 118 plates with limit 13.7 mag or fainter, 1928-1951; 3) recent very-wide-angle patrol series: 91 plates with limit 13.7 mag or fainter, 1968-1984; 4) other, non-patrol series: 100 plates with limit 13.7 mag or fainter, 1890-1944. Only three outbursts were detected, with data given in the table below. At other times the variable, when Table: Outbursts of the CV DO Dra Julian Date Mag (2,400,000+) (B) 28262.7 >12.2 invisible 28266.7 10.8: 28267.7 11.1 28273.7 >12.2 invisible 31498.7 >14.5 invisible 31499.7 >12.2 invisible 31504.7 10.0: 31505.8 10.8: 31506.7 11.2 31511.6 >12.2 invisible 31519.9 >13.7 invisible 33242.9 11.2 33279.8 >14.4 invisible seen on the plates, had magnitudes between 16 and 17, with occasional points brighter than 16 mag. Clearly, from the table, the outbursts are of short duration, lasting no more than ten days and probably even less. Thus, many outbursts would be quite easy to miss entirely. However, the number of outbursts observed, coupled with the number of plates searched, suggests that outbursts of this object are relatively infrequent. MARTHA L. HAZEN Harvard-Smithsonian Center for Astrophysics 60 Garden Street Cambridge, MA 02138 U.S.A.