Astrophysics (Index)About

eclipsing binary

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

An eclipsing binary is a binary star system in which one star passes in front of the other, detected by the reduction in observed light when that occurs, much as a transiting planet is detected. It is a type of variable star, with a variable type of E. 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 that is also a double-line spectroscopic binary and a detached binary (not in contact).


(star type,binary star type)
Further reading:
https://en.wikipedia.org/wiki/Eclipsing_binary

Referenced by pages:
Algol (Beta Per)
astrometric binary
binary star
contact binary
mass-luminosity relation
mass-radius relation
spectroscopic binary (SB)
spectrum binary
stellar mass determination
stellar parameter determination
stellar radius determination
STEREO
transient
variable star
visual binary
ZTF J1539+5027

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