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
LT AQL EA 12.4 – 14.9
MR AQL EA 15.0 – 16.0
OP AQL EA 12.2 – 14.6
QS AQL EA 5.93 – 6.0
QY AQL EA 11.4 – 14.6
V0340 AQL EA 11.5 – 14.1
V0342 AQL EA 9.5 – 12.9
V0343 AQL EA 10.6 – 12.3
V0346 AQL EA 9.0 – 10.1
V0348 AQL EA 13.0 – 14.5
V0406 AQL EA 13.1 – 15.5
V0407 AQL EA 13.3 – 15.8
V0408 AQL EA 14.1 – 16.5
V0409 AQL EA 11.5 – 12.4
V0413 AQL EA 13.7 – 15.8
V0414 AQL EA 14.0 – 15.7
V0415 AQL EA 11.1 – 12.0
V0416 AQL EA 13.7 – 15.1
V0418 AQL EA 12.8 – 16.0
V0420 AQL EA 12.8 – 14.3