Type of variability: EA

Algol (Beta Persei)-type eclipsing systems.

Binaries with spherical or slightly ellipsoidal components. It is possible to specify, for their light curves, the moments of the beginning and end of the eclipses. Between eclipses the light remains almost constant or varies insignificantly because of reflection effects, slight ellipsoidality of components, or physical variations. Secondary minima may be absent. An extremely wide range of periods is observed, from 0.2 to >= 10000 days. Light amplitudes are also quite different and may reach several magnitudes.

General Catalog of Variable Stars

4842

stars

0

observed in last month


Name Type Brightness
V0522 AND EA 13.34 – 13.9
V0523 AND EA 11.9 – 12.4
V0525 AND EA 11.2 – 11.5
V0537 AND EA 11.4 – 11.7
V0541 AND EA 12.58 – 13.4
V0543 AND EA 11.0 – 11.8
V0547 AND EA 11.38 – 11.7
V0560 AND EA 13.91 – 14.2
V0567 AND EA 11.65 – 12.3
V0581 AND EA 10.4 – 10.7
V0590 AND EA 13.05 – 13.4
V0591 AND EA 13.74 – 15.1
V0599 AND EA 12.7 – 13.0
V0601 AND EA 11.73 – 12.2
V0613 AND EA 9.15 – 9.6
V0629 AND EA 11.2 – 11.6
V0630 AND EA 14.4 – 15.1
V0643 AND EA 12.7 – 13.2
V0649 AND EA 11.55 – 11.7
V0651 AND EA 12.38 – 12.7