Curvaz de luz típicas  -  Typical light curves

(ASAS-3 data)

See that there's a progression in light curve shape between classes. The distinction between EA and EB is based primarily in the possibility of determination of the beginning and end of the eclipses. The distinction between EB and EW is based on the difference between minima I and II.

EA - Algol type

Per =  2.98328 d.

NSV 3682 - EA - 0.953865 d. - B7V	NSV 3877 - EA - 5.79935 d. - B5III	EZ Car - EA/KE - 1.1886887 d.- B4III-IV
V350 Cen - EA/KE: - 3.216915 d. -B3+B6	NSV 3812 - EA/KE - 3.17970 d. - OB	NSV 3645 - EA/KE - 2.54961 d. - A5
NSV 3687 - EB/KE - 0.688714 d. -A1/2V	NSV 5369 - EB/KE - 0.876112 d. - B5	NSV 7355 - EB - 3.18423 d. - O9.5IVn

EB - Beta Lyrae type

Per =  1.23501 d.

EW - W Ursae Majoris type

Per =  0.406614 d.

ESQUEMA EXPLICATIVO DE LOS ECLIPSES con V438 Pup y delta Velorum

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