Astrophysics (index)about

eclipsing binary

(E)
(binary star system detected by variations in magnitude)

An eclipsing binary is a binary star system where one star passes in front of the other, detected by seeing the change in light when that happens, much as a transiting planet is detected. In effect, it is a type of variable star, E commonly used as the variable type.

It is one of a number binary-star classes based upon how the star is determined to be binary. Others:

A double-line detached eclipsing binary (DDEB) is an eclipsing binary, a double-line spectroscopic binary and a detached binary (not touching).


(star type,binary star type)
http://en.wikipedia.org/wiki/Eclipsing_binary

Referenced by:
Algol (Beta Per)
astrometric binary
binary star
contact binary
mass-luminosity relation
mass-radius relation
spectroscopic binary
spectrum binary
stellar mass determination
stellar parameter determination
stellar radius determination
STEREO
variable star
visual binary

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