Type of variability: EB

Beta Lyrae-type eclipsing systems.

These are eclipsing systems having ellipsoidal components and light curves for which it is impossible to specify the exact times of onset and end of eclipses because of a continuous change of a system's apparent combined brightness between eclipses; secondary minimum is observed in all cases, its depth usually being considerably smaller than that of the primary minimum; periods are mainly longer than 1 day. The components generally belong to early spectral types (B-A). Light amplitudes are usually <2 mag in V.

General Catalog of Variable Stars

1149

stars

0

observed in last month


Name Type Brightness
AA AND EB 10.3 – 11.2
AD AND EB 11.2 – 11.8
AN AND EB 5.96 – 6.1
BD AND EB 11.3 – 11.7
BL AND EB 11.15 – 11.85
BX AND EB 8.87 – 9.5
CN AND EB 9.62 – 10.2
DO AND EB 12.3 – 13.8
LM AND EB 12.2 – 13.5
MN AND EB 15.1 – 16.2
PU AND EB 24.2 – 24.9
V0363 AND EB 9.1 – 9.3
V0376 AND EB 7.68 – 8.0
V0382 AND EB 9.16 – 9.4
V0406 AND EB 9.22 – 9.4
V0411 AND EB 15.0 – 16.1
V0422 AND EB 13.4 – 14.0
V0452 AND EB 13.7 – 15.2
V0463 AND EB 12.15 – 13.0
V0487 AND EB 11.6 – 11.7