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
V0348 AND EA 6.75 – 6.9
V0350 AND EA 7.56 – 7.6
V0355 AND EA 7.69 – 8.0
V0372 AND EA 9.05 – 9.5
V0377 AND EA 7.46 – 7.5
V0381 AND EA 7.35 – 7.4
V0389 AND EA 8.22 – 8.3
V0392 AND EA 9.07 – 9.4
V0404 AND EA 10.3 – 10.9
V0412 AND EA 11.95 – 12.4
V0413 AND EA 7.61 – 8.4
V0425 AND EA 13.3 – 14.6
V0440 AND EA 12.64 – 13.2
V0458 AND EA 12.2 – 12.8
V0462 AND EA 12.25 – 12.8
V0468 AND EA 10.9 – 11.5
V0496 AND EA 12.5 – 14.7
V0510 AND EA 13.9 – 14.5
V0512 AND EA 11.8 – 12.5
V0513 AND EA 12.8 – 13.2