Light Variations in Several Broad-Lined B Stars

M. Jerzykiewicz, C. Sterken
1982 Symposium - International astronomical union  
In our photoelectric searches for the β Cephei variables (JS77, JS79, and J82) several early B stars with nebulous lines were included. A summary of their photometric behaviour is presented in Table 1, columns four to six. Two of the stars, HR 2963 and HR 3476, areapparently constant in light , HR 3213 is a short-period β Cephei star, HR 3462 shews ellipsoidal variations with a period of Od.563, which implies an orbital period twice that long (cf. also Shobbrook 1981), and HR 8854 is an eclipsing binary with P = 2d.3913.
doi:10.1017/s0074180900037566 fatcat:bo5t5a35xrgdpbryav7aefdxda