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
V0445 AQL EA 13.0 – 15.5
V0479 AQL EA 13.2 – 14.6
V0494 AQL EA 14.4 – 16.1
V0495 AQL EA 14.5 – 15.0
V0557 AQL EA 13.4 – 15.6
V0589 AQL EA 14.7 – 16.4
V0602 AQL EA 11.9 – 13.2
V0611 AQL EA 14.2 – 15.3
V0616 AQL EA 14.1 – 15.0
V0630 AQL EA 14.3 – 16.0
V0631 AQL EA 13.5 – 14.9
V0634 AQL EA 14.8 – 16.2
V0644 AQL EA 14.8 – 16.2
V0647 AQL EA 14.7 – 15.6
V0688 AQL EA 10.3 – 11.1
V0690 AQL EA 15.1 – 15.7
V0694 AQL EA 12.4 – 12.9
V0711 AQL EA 15.0 – 16.1
V0712 AQL EA 14.4 – 14.8
V0714 AQL EA 13.9 – 14.8