COMMISSION 27 OF THE I. A. U.
        INFORMATION BULLETIN ON VARIABLE STARS
                     NUMBER 290

                                   Konkoly Observatory
                                   Budapest
                                   1968 July 19


                BV 449=BD -12d4227

This star was previously announced as an eclipsing binary having the period
0.^d49414 (1) and later 0.^d612077 (2).

Since spectroscopic observations collected at the Asiago Astrophysical
Observatory didn't agree with the above mentioned periods, photoelectric
observations have been made at the Observatory of the Bologna University. The
light curve shown below, results from the following elements:

Min I=JD 2439967.425+0.^d883036 E


                          [FIGURE 1]

                                        C. BARTOLINI
                                        P. BATTISTINI
                                        R. MARGONI
Asiago and Bologna
Astrophysical Observatories
July 12, 1968

(1) W. Strohmeier - IBVS, n. 62, 1964
(2) W. Strohmeier, R. Knigge, H. Ott - IBVS, n. 164, 1966.